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Bai L, Zou W, Wang L, Yu X, Lou H, Dai X, Teng W, Yu W, Li M, Cao H, Zheng L. Effect of "Tiaoshen" acupuncture technique on mild depression and its underlying mechanism: A randomized controlled trial study protocol. Heliyon 2024; 10:e28889. [PMID: 38596088 PMCID: PMC11002658 DOI: 10.1016/j.heliyon.2024.e28889] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/24/2023] [Revised: 03/14/2024] [Accepted: 03/26/2024] [Indexed: 04/11/2024] Open
Abstract
Background Mild depression is not just a mental disease, but also a serious and long-term public health issue. It affects the quality of life of patients and can quickly develop into major depression. There are currently no effective drug treatments with high efficacy and few adverse reactions. Acupuncture may be an alternative treatment option. Preliminary experiments and practices have demonstrated that "Tiaoshen" acupuncture improves symptoms in patients who have depression, however the underlying data and method remain unclear at present. Methods This is a prospective, single-center, single-blind, randomized controlled trial. We plan to recruit 70 participants and randomly assign them to receive "Tiaoshen" acupuncture or traditional acupuncture at a ratio of 1:1. Then, all the participants will receive the appropriate acupuncture treatment for four weeks. The results of the Hamilton Depression Rating Scale (HDSR-24) will serve as the primary outcome, while the results of the Patient Health Questionnaire-9 (PHQ-9) and the World Health Organization Quality of Life Brief Version (WHOQOL-BREF) will serve as secondary outcomes. Evaluations will be conducted at baseline, 1, 2, and 4 weeks after treatment initiation, and 1 and 3 months after treatment completion. The safety of the intervention will be evaluated every week using the Columbia-Suicide Severity Rating Scale (C-SSRS) and the Treatment Emergent Symptoms Scale (TESS). Serum levels of oxidative stress markers 8-iso-prostaglandin F2α (8-iso-PGF2α), superoxide dismutase (SOD), uric acid (UA), and total bilirubin (TBIL) will be measured at baseline and the end of the treatment. We will conduct a statistical analysis of intention to treat (ITT) and conformance to protocol set (PPS) data. Discussion This research aims to provide high-quality evidence for the efficacy and safety of "Tiaoshen" acupuncture as a treatment for mild depression. In addition, the mechanism through which acupuncture heals mild depression will be investigated.
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Affiliation(s)
- Lu Bai
- Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Wei Zou
- The third department of Acupuncture, the First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
- Clinical Key Laboratory of Integrated Traditional Chinese and Western Medicine, Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Long Wang
- The first Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Xueping Yu
- The third department of Acupuncture, the First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Hongjun Lou
- The first Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Xiaohong Dai
- Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Wei Teng
- Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Weiwei Yu
- The third department of Acupuncture, the First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Mingyue Li
- The third department of Acupuncture, the First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Hongtao Cao
- The third department of Acupuncture, the First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
| | - Lei Zheng
- The third department of Acupuncture, the First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, 150040, China
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Wang R, Lin Y', Zhang C, Wu H, Jin Q, Guo J, Cao H, Tan D, Wu T. Fine mapping and analysis of a candidate gene controlling Phytophthora blight resistance in cucumber. Plant Biol (Stuttg) 2024. [PMID: 38607927 DOI: 10.1111/plb.13648] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/15/2023] [Accepted: 03/25/2024] [Indexed: 04/14/2024]
Abstract
Cucumber blight is a destructive disease. The best way to control this disease is resistance breeding. This study focuses on disease resistance gene mapping and molecular marker development. We used the resistant cucumber, JSH, and susceptible cucumber, B80, as parents to construct F2 populations. Bulked segregant analysis (BSA) combined with specific length amplified fragment sequencing (SLAF-seq) were used, from which we developed cleaved amplified polymorphic sequence (CAPs) markers to map the resistance gene. Resistance in F2 individuals showed a segregation ratio of resistance:susceptibility close to 3:1. The gene in JSH resistant cucumber was mapped to an interval of 9.25 kb, and sequencing results for the three genes in the mapped region revealed three mutations at base sites 225, 302, and 591 in the coding region of Csa5G139130 between JSH and B80, but no mutations in coding regions of Csa5G139140 and Csa5G139150. The mutations caused changes in amino acids 75 and 101 of the protein encoded by Csa5G139130, suggesting that Csa5G139130 is the most likely resistance candidate gene. We developed a molecular marker, CAPs-4, as a closely linked marker for the cucumber blight resistance gene. This is the first report on mapping of a cucumber blight resistance gene and will provideg a useful marker for molecular breeding of cucumber resistance to Phytophthora blight.
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Affiliation(s)
- R Wang
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
| | - Y 'e Lin
- Vegetable Research Institute, Guangdong Academy of Agricultural Sciences/Guangdong Key Laboratory for New Technology Research of Vegetables, Guangzhou, China
| | - C Zhang
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
| | - H Wu
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
| | - Q Jin
- Vegetable Research Institute, Guangdong Academy of Agricultural Sciences/Guangdong Key Laboratory for New Technology Research of Vegetables, Guangzhou, China
| | - J Guo
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
| | - H Cao
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
| | - D Tan
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
| | - T Wu
- Institute of Facility Agriculture, Guangdong Academy of Agricultural Sciences (IFA, GDAAS), Guangzhou, China
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Fu X, Li K, Zhang C, Wang Q, Xu G, Rogachev AA, Yarmolenko MA, Cao H, Zhang H. Homogeneous and Nanogranular Prussian Blue to Enable Long-Term-Stable Electrochromic Devices. ACS Appl Mater Interfaces 2024; 16:17745-17756. [PMID: 38523600 DOI: 10.1021/acsami.3c17551] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 03/26/2024]
Abstract
The increasing demand for the state-of-the-art electrochromic devices has received great interest in synthesizing Prussian blue (PB) nanoparticles with a uniform diameter that exhibit excellent electrochromism, electrochemistry, and cyclability. Herein, we report the controllable synthesis of sub-100 nm PB nanoparticles via the coprecipitation method. The diameter of PB nanoparticles can be modulated by adjusting the reactant concentration, the selection of a chelator, and their purification. The self-assembled nanogranular thin films, homogeneously fabricated by using optimized PB nanoparticles with an average diameter of 50 nm as building blocks via the blade coating technique enable excellent performance with a large optical modulation of 80% and a high coloration efficiency of 417.79 cm2 C-1. It is also demonstrated by in situ and ex situ observations that the nanogranular PB thin films possess outstanding structural and electrochemical reversibility. Furthermore, such nanogranular PB thin films can enjoy the enhanced long-term cycling stability of the PB-WO3 complementary electrochromic devices having a 91.4% optical contrast retention after 16,000 consecutive cycles. This work provides a newly and industrially compatible approach to producing a complementary electrochromic device with extraordinary durability for various practical applications.
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Affiliation(s)
- Xiaofang Fu
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, PR China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, PR China
| | - Kun Li
- Vallight Optics Technology Ningbo Co., Ltd, Ningbo 315400, PR China
| | - Chengli Zhang
- Ningbo Wakan Electronic Science Technology Co., Ltd, Ningbo 315475, PR China
| | - Qiang Wang
- Ningbo Wakan Electronic Science Technology Co., Ltd, Ningbo 315475, PR China
| | - Guanglong Xu
- Ningbo Wakan Electronic Science Technology Co., Ltd, Ningbo 315475, PR China
| | - Alexander Alexandrovich Rogachev
- Optical Anisotropic Films Laboratory, Institute of Chemistry of New Materials of the National Academy of Sciences of Belarus, Minsk 220141, Belarus
| | | | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, PR China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, PR China
| | - Hongliang Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, PR China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, PR China
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Cao H, Hansen LM, Giorgino F, Carosini L, Zahálka P, Zilk F, Loredo JC, Walther P. Photonic Source of Heralded Greenberger-Horne-Zeilinger States. Phys Rev Lett 2024; 132:130604. [PMID: 38613278 DOI: 10.1103/physrevlett.132.130604] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/10/2023] [Accepted: 02/22/2024] [Indexed: 04/14/2024]
Abstract
Generating large multiphoton entangled states is of main interest due to enabling universal photonic quantum computing and all-optical quantum repeater nodes. These applications exploit measurement-based quantum computation using cluster states. Remarkably, it was shown that photonic cluster states of arbitrary size can be generated by using feasible heralded linear optics fusion gates that act on heralded three-photon Greenberger-Horne-Zeilinger (GHZ) states as the initial resource state. Thus, the capability of generating heralded GHZ states is of great importance for scaling up photonic quantum computing. Here, we experimentally demonstrate this required building block by reporting a polarisation-encoded heralded GHZ state of three photons, for which we build a high-rate six-photon source (547±2 Hz) from a solid-state quantum emitter and a stable polarization-based interferometer. The detection of three ancillary photons heralds the generation of three-photon GHZ states among the remaining particles with fidelities up to F=0.7278±0.0106. Our results initiate a path for scalable entangling operations using heralded linear-optics implementations.
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Affiliation(s)
- H Cao
- University of Vienna, Faculty of Physics, Vienna Center for Quantum Science and Technology (VCQ), 1090 Vienna, Austria
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - L M Hansen
- University of Vienna, Faculty of Physics, Vienna Center for Quantum Science and Technology (VCQ), 1090 Vienna, Austria
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - F Giorgino
- University of Vienna, Faculty of Physics, Vienna Center for Quantum Science and Technology (VCQ), 1090 Vienna, Austria
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - L Carosini
- University of Vienna, Faculty of Physics, Vienna Center for Quantum Science and Technology (VCQ), 1090 Vienna, Austria
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - P Zahálka
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - F Zilk
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - J C Loredo
- University of Vienna, Faculty of Physics, Vienna Center for Quantum Science and Technology (VCQ), 1090 Vienna, Austria
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
| | - P Walther
- University of Vienna, Faculty of Physics, Vienna Center for Quantum Science and Technology (VCQ), 1090 Vienna, Austria
- Christian Doppler Laboratory for Photonic Quantum Computer, Faculty of Physics, University of Vienna, 1090 Vienna, Austria
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Shan JT, Hua ZH, Xu P, Cao H, Jiao ZY, Sun LK, Liu SR, Xia L, Xue WH, Li Z. [Mid- and long-term results of surgical treatment of brachiocephalic Takayasu arteritis]. Zhonghua Wai Ke Za Zhi 2024; 62:229-234. [PMID: 38291639 DOI: 10.3760/cma.j.cn112139-20230904-00090] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Subscribe] [Scholar Register] [Indexed: 02/01/2024]
Abstract
Objective: To examine the mid - and long-term outcomes of surgical treatment of brachiocephalic Takayasu arteritis. Methods: This is a retrospective case series study. The clinical data of 39 patients,which had been diagnosed as brachiocephalic Takayasu arteritis (244 cases),who underwent surgical treatment,were analyzed between July 2012 to November 2022 at Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University. There were 5 males and 34 females, aged (37.9±14.0)years (range:13 to 71 years). Despite medical treatment, the patients suffered severe ischemic symptoms continually and then underwent surgical interventions. Among them, 20 patients underwent endovascular procedures, 11 underwent open surgical procedures, and 8 underwent hybrid procedures. Patients were followed up through outpatient visits at 1, 3, 6 months after surgery and once every year later. Follow-up was conducted until November 2022. Operation status, postoperative complications and re-intervention of patients were recorded and the Kaplan-Meier survival curves were used to analyze postoperative vascular patency rates. Results: All 39 surgeries were successful, with no intraoperative death or serious complications. The follow-up period was (48.8±38.2) months(range:1 to 123 months). Thirty-three patients experienced symptom relief after surgery, and 6 patients required secondary surgical interventions. The patency rates for the endovascular treatment group at 1-, 3-, 5-, and 10-year were 95.0%, 75.2%, 60.2%, and 60.2%, respectively, while the patency rates for open surgery were all 90.9%. In the hybrid surgery group, the patency rates at 1-, 3-, 5-, and 8-year were all 87.5%. Conclusion: For patients with brachiocephalic Takayasu arteritis, choice of an appropriate blood flow revascularization intervention should be based on the patient's condition,and the mid-and long-term outcomes are satisfactory.
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Affiliation(s)
- J T Shan
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - Z H Hua
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - P Xu
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - H Cao
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - Z Y Jiao
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - L K Sun
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - S R Liu
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - L Xia
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - W H Xue
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
| | - Z Li
- Department of Endoluminal Vascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450000, China
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Zhang ZZ, Zhu CC, Cao H. [Thinking and strategy selection on the quality control of early gastric cancer]. Zhonghua Wei Chang Wai Ke Za Zhi 2024; 27:137-142. [PMID: 38413079 DOI: 10.3760/cma.j.cn441530-20231101-00153] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Subscribe] [Scholar Register] [Indexed: 02/29/2024]
Abstract
With the developing technique of the diagnosis and treatment of early gastric cancer, the quality of early gastric cancer diagnosis and treatment is coming into focus, and is crucial to improve the overall management of gastric cancer. It is necessary to establish a quality control system to ensure the quality of diagnosis and treatment for EGC. Based on the summary of the diagnosis and treatment status and technological progress of early gastric cancer, this paper proposes the quality control strategy, content and plan for the diagnosis and treatment process of EGC from the aspects of multidisciplinary diagnosis and treatment, clinical diagnosis technology, endoscopic and surgical treatment, pathological diagnosis and follow-up, with a view to expound the rationality, standardization and quality guarantee of the diagnosis and treatment process for early gastric cancer.
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Affiliation(s)
- Z Z Zhang
- Department of Gastrointestinal Surgery, Ren Ji Hospital, Shanghai Jiao Tong University School of Medicine, Shanghai 200127, China
| | - C C Zhu
- Department of Gastrointestinal Surgery, Ren Ji Hospital, Shanghai Jiao Tong University School of Medicine, Shanghai 200127, China
| | - H Cao
- Department of Gastrointestinal Surgery, Ren Ji Hospital, Shanghai Jiao Tong University School of Medicine, Shanghai 200127, China
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Zhang C, Zheng J, Yu X, Kuang B, Dai X, Zheng L, Yu W, Teng W, Cao H, Li M, Yao J, Liu X, Zou W. "Baihui" (DU20)-penetrating "Qubin" (GB7) acupuncture on blood-brain barrier integrity in rat intracerebral hemorrhage models via the RhoA/ROCK II/MLC 2 signaling pathway. Animal Model Exp Med 2024. [PMID: 38379356 DOI: 10.1002/ame2.12374] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/28/2023] [Accepted: 11/21/2023] [Indexed: 02/22/2024] Open
Abstract
BACKGROUND Blocking the RhoA/ROCK II/MLC 2 (Ras homolog gene family member A/Rho kinase II/myosin light chain 2) signaling pathway can initiate neuroprotective mechanisms against neurological diseases such as stroke, cerebral ischemia, and subarachnoid hemorrhage. Nevertheless, it is not clear whether and how disrupting the RhoA/ROCK II/MLC 2 signaling pathway changes the pathogenic processes of the blood-brain barrier (BBB) after intracerebral hemorrhage (ICH). The present investigation included the injection of rat caudal vein blood into the basal ganglia area to replicate the pathophysiological conditions caused by ICH. METHODS Scalp acupuncture (SA) therapy was performed on rats with ICH at the acupuncture point "Baihui"-penetrating "Qubin," and the ROCK selective inhibitor fasudil was used as a positive control to evaluate the inhibitory effect of acupuncture on the RhoA/ROCK II/MLC 2 signaling pathway. Post-assessments included neurological deficits, brain edema, Evans blue extravasation, Western blot, quantitative polymerase chain reaction, and transmission electron microscope imaging. RESULTS We found that ROCK II acts as a promoter of the RhoA/ROCK II/MLC 2 signaling pathway, and its expression increased at 6 h after ICH, peaked at 3 days, and then decreased at 7 days after ICH, but was still higher than the pre-intervention level. According to some experimental results, although 3 days is the peak, 7 days is the best time point for acupuncture treatment. Starting from 6 h after ICH, the neurovascular structure and endothelial cell morphology around the hematoma began to change. Based on the changes in the promoter ROCK II, a 7-day time point was selected as the breakthrough point for treating ICH model rats in the main experiment. The results of this experiment showed that both SA at "Baihui"-penetrating "Qubin" and treatment with fasudil could improve the expression of endothelial-related proteins by inhibiting the RhoA/ROCK II/MLC 2 signaling pathway and reduce neurological dysfunction, brain edema, and BBB permeability in rats. CONCLUSION This study found that these experimental data indicated that SA at "Baihui"-penetrating "Qubin" could preserve BBB integrity and neurological function recovery after ICH by inhibiting RhoA/ROCK II/MLC 2 signaling pathway activation and by regulating endothelial cell-related proteins.
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Affiliation(s)
- Ce Zhang
- Heilongjiang University of Chinese Medicine, Harbin, China
| | - Jia Zheng
- Heilongjiang University of Chinese Medicine, Harbin, China
| | - Xueping Yu
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Binglin Kuang
- Heilongjiang University of Chinese Medicine, Harbin, China
| | - Xiaohong Dai
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Lei Zheng
- Clinical Key Laboratory of Integrated Traditional Chinese and Western Medicine of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Weiwei Yu
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Wei Teng
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Hongtao Cao
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Mingyue Li
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Jiayong Yao
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Xiaoying Liu
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
| | - Wei Zou
- First Affiliated Hospital of Heilongjiang University of Chinese Medicine, Harbin, China
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Zhou BN, Hua ZH, Xia L, Cao H, Jiao ZY, Xu P, Zhang S, Zhang Q, Li Z. [Clinical characteristics and efficacy analysis of various treatments for spontaneous carotid artery dissection]. Zhonghua Yi Xue Za Zhi 2024; 104:337-343. [PMID: 38281801 DOI: 10.3760/cma.j.cn112137-20231007-00645] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Subscribe] [Scholar Register] [Indexed: 01/30/2024]
Abstract
Objective: To investigate the clinical features of spontaneous carotid artery dissection (SCAD) and the efficacy of different treatment methods. Methods: The clinical data of 164 patients with SCAD who were treated at the First Affiliated Hospital of Zhengzhou University from June 2018 to January 2023 were retrospectively analyzed. There were 127 males and 37 females, with a mean age of (49.5±11.1) years. They were divided into conservative treatment group (n=100) and surgical treatment group (n=64) according to whether they received surgical treatment. Patients were followed at 3, 6, and 12 months after discharge and annually thereafter through outpatient or inpatient visits. The incidence of cerebral ischemic events, cerebral hemorrhage events, and mortality rates during hospitalization and follow-up periods were analyzed in the two patient groups. To examine correlates of revascularization in SCAD, multifactorial logistic regression analysis was used. Results: Of the 164 patients, 18 patients had bilateral SCAD and a total of 182 carotid arteries were included in the study. Ischemic stroke (85 cases, 51.8%) and transient ischemic attack (31 cases, 18.9%) were the main clinical manifestations in SCAD patients. Hypertension (81 cases, 49.4%) and hyperlipidemia (39 cases, 23.8%) were the main comorbidities in SCAD patients. During hospitalization, 100 patients in the conservative treatment group received medication in 113 carotid arteries, no new cerebral ischemic events or symptomatic intracranial hemorrhage events occurred, and no death occurred. A total of 69 carotid arteries were surgically treated in 64 patients in the surgical treatment group. The success rate was 97.1% (67/69). In the surgical treatment group, the proportion of carotid stenosis degree≥90% was 47.8% (33/69), the proportion of type Ⅱ SCAD was 60.9% (42/69), and the proportion discharged from the hospital to receive antiplatelet therapy was 92.8% (64/69), which were higher than those in the conservative treatment group, which were 25.7% (29/113), 45.1% (51/113), and 73.5% (83/113), respectively (all P<0.05). The follow-up time [M(Q1, Q3)] in the conservative treatment group was 24 (13, 34) months, with an 8% (9/113) rate of ischemic events and a 7.1% (8/113) rate of readmission; in the surgical treatment group, the follow-up time was 24 (11, 38) months, and there were no new ischemic events or deaths. The results of multifactorial logistic regression analysis showed that the degree of true luminal stenosis<90% (OR=2.738, 95%CI: 1.067-7.026, P=0.036) and type Ⅰ dissections (OR=2.656, 95%CI: 1.189-5.935, P=0.017) were the correlates of complete revascularization. Conclusions: Ischemic stroke and transient ischemic attack are the main clinical manifestations in patients with SCAD. Pharmacological antithrombotic therapy remains the method of choice, and endovascular treatment after failure of conservative therapy reduces the risk of recurrent long-term cerebral ischemic events and the re-admission rate of patients.
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Affiliation(s)
- B N Zhou
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - Z H Hua
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - L Xia
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - H Cao
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - Z Y Jiao
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - P Xu
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - S Zhang
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - Q Zhang
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
| | - Z Li
- Department of Endovascular Surgery, the First Affiliated Hospital of Zhengzhou University, Zhengzhou 450052, China
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Gao Z, Zhang C, Wang Q, Xu G, Gao J, Cao H, Zhang H. Improved Electrical Resistivity of Atomic-Layer-Deposited Copper Thin Films on Polyimide Substrates by an In Situ ZnO Interlayer. ACS Appl Mater Interfaces 2024; 16:1876-1882. [PMID: 38113383 DOI: 10.1021/acsami.3c15182] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/21/2023]
Abstract
The low-temperature atomic layer deposition of metal on polymer surfaces is often challenging owing to the deficiency of functional groups and reactivity. Here, the deposition of ALD-Cu employing Cu(hfac)2 and Et2Zn at a low temperature (120 °C) on polyimide (PI) substrates is improved by the utilization of an in situ ultrathin ALD-ZnO buffer layer. A conformal and continuous ALD-Cu thin film with low resistivity (6.07 μΩ cm) is fabricated on an ALD-ZnO/PI substrate. The findings demonstrate that the ALD-ZnO buffer layer provides chemisorption and a nucleation site for the initial growth of ALD-Cu. Transmission electron microscopy and energy-dispersive X-ray analysis reveal that the ALD-ZnO layer plays a buffer role in the fitness of ALD-Cu on PI substrates and its ability to elicit the formation of an ALD-ZnO nanocluster and polar surface. ALD-ZnO can be effectively utilized as a buffer layer for polymer-based ALD-metal processes, showing potential in flexible electronic applications.
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Affiliation(s)
- Zihong Gao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, Zhejiang 315201, People's Republic of China
| | - Chengli Zhang
- Ningbo Wakan Electronic Science Technology Company, Limited, Ningbo, Zhejiang 315475, People's Republic of China
| | - Qiang Wang
- Ningbo Wakan Electronic Science Technology Company, Limited, Ningbo, Zhejiang 315475, People's Republic of China
| | - Guanglong Xu
- Ningbo Wakan Electronic Science Technology Company, Limited, Ningbo, Zhejiang 315475, People's Republic of China
| | - Junhua Gao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, Zhejiang 315201, People's Republic of China
| | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, Zhejiang 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
| | - Hongliang Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, Zhejiang 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
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Effects of empagliflozin on progression of chronic kidney disease: a prespecified secondary analysis from the empa-kidney trial. Lancet Diabetes Endocrinol 2024; 12:39-50. [PMID: 38061371 PMCID: PMC7615591 DOI: 10.1016/s2213-8587(23)00321-2] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 09/05/2023] [Revised: 10/24/2023] [Accepted: 10/25/2023] [Indexed: 12/23/2023]
Abstract
BACKGROUND Sodium-glucose co-transporter-2 (SGLT2) inhibitors reduce progression of chronic kidney disease and the risk of cardiovascular morbidity and mortality in a wide range of patients. However, their effects on kidney disease progression in some patients with chronic kidney disease are unclear because few clinical kidney outcomes occurred among such patients in the completed trials. In particular, some guidelines stratify their level of recommendation about who should be treated with SGLT2 inhibitors based on diabetes status and albuminuria. We aimed to assess the effects of empagliflozin on progression of chronic kidney disease both overall and among specific types of participants in the EMPA-KIDNEY trial. METHODS EMPA-KIDNEY, a randomised, controlled, phase 3 trial, was conducted at 241 centres in eight countries (Canada, China, Germany, Italy, Japan, Malaysia, the UK, and the USA), and included individuals aged 18 years or older with an estimated glomerular filtration rate (eGFR) of 20 to less than 45 mL/min per 1·73 m2, or with an eGFR of 45 to less than 90 mL/min per 1·73 m2 with a urinary albumin-to-creatinine ratio (uACR) of 200 mg/g or higher. We explored the effects of 10 mg oral empagliflozin once daily versus placebo on the annualised rate of change in estimated glomerular filtration rate (eGFR slope), a tertiary outcome. We studied the acute slope (from randomisation to 2 months) and chronic slope (from 2 months onwards) separately, using shared parameter models to estimate the latter. Analyses were done in all randomly assigned participants by intention to treat. EMPA-KIDNEY is registered at ClinicalTrials.gov, NCT03594110. FINDINGS Between May 15, 2019, and April 16, 2021, 6609 participants were randomly assigned and then followed up for a median of 2·0 years (IQR 1·5-2·4). Prespecified subgroups of eGFR included 2282 (34·5%) participants with an eGFR of less than 30 mL/min per 1·73 m2, 2928 (44·3%) with an eGFR of 30 to less than 45 mL/min per 1·73 m2, and 1399 (21·2%) with an eGFR 45 mL/min per 1·73 m2 or higher. Prespecified subgroups of uACR included 1328 (20·1%) with a uACR of less than 30 mg/g, 1864 (28·2%) with a uACR of 30 to 300 mg/g, and 3417 (51·7%) with a uACR of more than 300 mg/g. Overall, allocation to empagliflozin caused an acute 2·12 mL/min per 1·73 m2 (95% CI 1·83-2·41) reduction in eGFR, equivalent to a 6% (5-6) dip in the first 2 months. After this, it halved the chronic slope from -2·75 to -1·37 mL/min per 1·73 m2 per year (relative difference 50%, 95% CI 42-58). The absolute and relative benefits of empagliflozin on the magnitude of the chronic slope varied significantly depending on diabetes status and baseline levels of eGFR and uACR. In particular, the absolute difference in chronic slopes was lower in patients with lower baseline uACR, but because this group progressed more slowly than those with higher uACR, this translated to a larger relative difference in chronic slopes in this group (86% [36-136] reduction in the chronic slope among those with baseline uACR <30 mg/g compared with a 29% [19-38] reduction for those with baseline uACR ≥2000 mg/g; ptrend<0·0001). INTERPRETATION Empagliflozin slowed the rate of progression of chronic kidney disease among all types of participant in the EMPA-KIDNEY trial, including those with little albuminuria. Albuminuria alone should not be used to determine whether to treat with an SGLT2 inhibitor. FUNDING Boehringer Ingelheim and Eli Lilly.
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T, Tamori Y, Tamura R, Tamura Y, Tan CHH, Tan EZZ, Tanabe A, Tanabe K, Tanaka A, Tanaka A, Tanaka N, Tang S, Tang Z, Tanigaki K, Tarlac M, Tatsuzawa A, Tay JF, Tay LL, Taylor J, Taylor K, Taylor K, Te A, Tenbusch L, Teng KS, Terakawa A, Terry J, Tham ZD, Tholl S, Thomas G, Thong KM, Tietjen D, Timadjer A, Tindall H, Tipper S, Tobin K, Toda N, Tokuyama A, Tolibas M, Tomita A, Tomita T, Tomlinson J, Tonks L, Topf J, Topping S, Torp A, Torres A, Totaro F, Toth P, Toyonaga Y, Tripodi F, Trivedi K, Tropman E, Tschope D, Tse J, Tsuji K, Tsunekawa S, Tsunoda R, Tucky B, Tufail S, Tuffaha A, Turan E, Turner H, Turner J, Turner M, Tuttle KR, Tye YL, Tyler A, Tyler J, Uchi H, Uchida H, Uchida T, Uchida T, Udagawa T, Ueda S, Ueda Y, Ueki K, Ugni S, Ugwu E, Umeno R, Unekawa C, Uozumi K, Urquia K, Valleteau A, Valletta C, van Erp R, Vanhoy C, Varad V, Varma R, Varughese A, Vasquez P, Vasseur A, Veelken R, Velagapudi C, Verdel K, Vettoretti S, Vezzoli G, Vielhauer V, Viera R, Vilar E, Villaruel S, 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Yamada N, Yamagata K, Yamaguchi M, Yamaji Y, Yamamoto A, Yamamoto S, Yamamoto S, Yamamoto T, Yamanaka A, Yamano T, Yamanouchi Y, Yamasaki N, Yamasaki Y, Yamasaki Y, Yamashita C, Yamauchi T, Yan Q, Yanagisawa E, Yang F, Yang L, Yano S, Yao S, Yao Y, Yarlagadda S, Yasuda Y, Yiu V, Yokoyama T, Yoshida S, Yoshidome E, Yoshikawa H, Young A, Young T, Yousif V, Yu H, Yu Y, Yuasa K, Yusof N, Zalunardo N, Zander B, Zani R, Zappulo F, Zayed M, Zemann B, Zettergren P, Zhang H, Zhang L, Zhang L, Zhang N, Zhang X, Zhao J, Zhao L, Zhao S, Zhao Z, Zhong H, Zhou N, Zhou S, Zhu D, Zhu L, Zhu S, Zietz M, Zippo M, Zirino F, Zulkipli FH. Impact of primary kidney disease on the effects of empagliflozin in patients with chronic kidney disease: secondary analyses of the EMPA-KIDNEY trial. Lancet Diabetes Endocrinol 2024; 12:51-60. [PMID: 38061372 DOI: 10.1016/s2213-8587(23)00322-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 09/05/2023] [Revised: 10/24/2023] [Accepted: 10/25/2023] [Indexed: 12/23/2023]
Abstract
BACKGROUND The EMPA-KIDNEY trial showed that empagliflozin reduced the risk of the primary composite outcome of kidney disease progression or cardiovascular death in patients with chronic kidney disease mainly through slowing progression. We aimed to assess how effects of empagliflozin might differ by primary kidney disease across its broad population. METHODS EMPA-KIDNEY, a randomised, controlled, phase 3 trial, was conducted at 241 centres in eight countries (Canada, China, Germany, Italy, Japan, Malaysia, the UK, and the USA). Patients were eligible if their estimated glomerular filtration rate (eGFR) was 20 to less than 45 mL/min per 1·73 m2, or 45 to less than 90 mL/min per 1·73 m2 with a urinary albumin-to-creatinine ratio (uACR) of 200 mg/g or higher at screening. They were randomly assigned (1:1) to 10 mg oral empagliflozin once daily or matching placebo. Effects on kidney disease progression (defined as a sustained ≥40% eGFR decline from randomisation, end-stage kidney disease, a sustained eGFR below 10 mL/min per 1·73 m2, or death from kidney failure) were assessed using prespecified Cox models, and eGFR slope analyses used shared parameter models. Subgroup comparisons were performed by including relevant interaction terms in models. EMPA-KIDNEY is registered with ClinicalTrials.gov, NCT03594110. FINDINGS Between May 15, 2019, and April 16, 2021, 6609 participants were randomly assigned and followed up for a median of 2·0 years (IQR 1·5-2·4). Prespecified subgroupings by primary kidney disease included 2057 (31·1%) participants with diabetic kidney disease, 1669 (25·3%) with glomerular disease, 1445 (21·9%) with hypertensive or renovascular disease, and 1438 (21·8%) with other or unknown causes. Kidney disease progression occurred in 384 (11·6%) of 3304 patients in the empagliflozin group and 504 (15·2%) of 3305 patients in the placebo group (hazard ratio 0·71 [95% CI 0·62-0·81]), with no evidence that the relative effect size varied significantly by primary kidney disease (pheterogeneity=0·62). The between-group difference in chronic eGFR slopes (ie, from 2 months to final follow-up) was 1·37 mL/min per 1·73 m2 per year (95% CI 1·16-1·59), representing a 50% (42-58) reduction in the rate of chronic eGFR decline. This relative effect of empagliflozin on chronic eGFR slope was similar in analyses by different primary kidney diseases, including in explorations by type of glomerular disease and diabetes (p values for heterogeneity all >0·1). INTERPRETATION In a broad range of patients with chronic kidney disease at risk of progression, including a wide range of non-diabetic causes of chronic kidney disease, empagliflozin reduced risk of kidney disease progression. Relative effect sizes were broadly similar irrespective of the cause of primary kidney disease, suggesting that SGLT2 inhibitors should be part of a standard of care to minimise risk of kidney failure in chronic kidney disease. FUNDING Boehringer Ingelheim, Eli Lilly, and UK Medical Research Council.
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Fu X, Zhang Z, Cao Z, Rogachev AA, Yarmolenko MA, Chen T, Cao H, Zhang H. Mechanistic Insights into Anion-Induced Electrochromism of Ru(II)-Based Metallo-Supramolecular Polymer. Polymers (Basel) 2023; 15:4735. [PMID: 38139986 PMCID: PMC10747135 DOI: 10.3390/polym15244735] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/21/2023] [Revised: 12/14/2023] [Accepted: 12/15/2023] [Indexed: 12/24/2023] Open
Abstract
The metallo-supramolecular polymer (MSP) is considered one of the most promising electrodes for electrochromic devices due to its intrinsically stable redox properties. Nevertheless, despite extensive work focusing on improving the electrochromic and electrochemical properties of MSPs, little experimental evidence exists from in-depth investigations on the anion-induced electrochromism of MSPs. Herein, Ru-based metallo-supramolecular polymer (polyRu) films with excellent electrochromic performance were fabricated through a novel electrochemical deposition method, and the electrochromic mechanism was further understood. The polyRu films possess fast reaction kinetics with a short switching time of 4.0 s (colored) and 2.8 s (bleached) and highly reversible redox properties due to the resulting impacts on the capacitive behaviors (containing surface, near-surface and intercalation pseudo-capacitance) of the perchlorate ions in the electrochromic process. Moreover, the electrochromic degradation of the polyRu films is considered to stem from the numerous nanopores in the film induced by ClO4- transport and the exchange of counter anions from Cl- to ClO4-. In addition, a physical model, revealing the transport of conduction ions and the evolution of the structure and properties of the polyRu film during the electrochromic process, is presented. It is observed that the charge balance of Ru3+ and Ru2+, achieved through the adsorption/desorption of ClO4- on the film, provides electrochromic and electrochemical reversibility to the polyRu film under positive/negative bias. Correspondingly, a transformation from polyRu·(Cl-)2n to polyRu·(ClO4-)x(Cl-)2n-x in the polyRu film is induced by a counter anion exchange from Cl- to ClO4-. Revealing the detailed perchlorate ion transfer kinetics and electrochromic mechanism in this film can offer new insights into the application of metallo-supramolecular polymers in electrochromic devices.
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Affiliation(s)
- Xiaofang Fu
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China (H.C.)
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Zhuohui Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China (H.C.)
- Nano Science and Technology Institute, University of Science and Technology of China, Suzhou 215123, China
| | - Zhenhu Cao
- Ningbo Mi Ruo Electronic Technology Co., Ltd., Ningbo 315203, China
| | - Alexandr Alexandrovich Rogachev
- Optical Anisotropic Films Laboratory, Institute of Chemistry of New Materials of the National Academy of Sciences of Belarus, 220141 Minsk, Belarus
| | - Maxim Anatolievich Yarmolenko
- Department of Radiophysics and Electronics, Francisk Skorina Gomel State University, 104, Sovetskaya Street, 246019 Gomel, Belarus
| | - Tao Chen
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China (H.C.)
| | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China (H.C.)
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Hongliang Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China (H.C.)
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
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Cao H, Zhang S, Zheng X, Xu L, Diao J, Wang Y, Gai C, Ye H. Safety assessment of Rhodobacter azotoformans SY5 for potential application in Chinese mitten crab Eriocheir sinensis. Benef Microbes 2023; 14:641-651. [PMID: 38350469 DOI: 10.1163/18762891-20230086] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/11/2023] [Accepted: 11/02/2023] [Indexed: 02/15/2024]
Abstract
Rhodobacter species are promising beneficial microbes that can improve growth performance, immunity and antioxidant capability in aquatic crustaceans. Yet the safety of Rhodobacter azotoformans for potential application in Chinese mitten crab Eriocheir sinensis is still unclear. In the present study, R. azotoformans SY5, a potential probiotic additive that can significantly improve the growth performance, immunity, antioxidant capability, and disease resistance in E. sinensis, was evaluated for safety through whole genome sequencing, antibiotic resistance, toxic metabolites, virulence, and crab tolerance assays. The results indicated that R. azotoformans SY5 only harboured the acyl carrier protein-encoding gene (acpP) that was universal in probiotic bacteria with the function of bacterial fatty acid biosynthesis, exhibited high susceptibility to aminoglycosides, penicillins, polymyxins, polyphosphates, quinolones, and tetracyclines antimicrobials, and possessed inability to produce hemolysin, hydrogen sulphide, nitrite, ammonia, and phenylpyruvate. In addition, R. azotoformans SY5 showed no pathogenicity for E. sinensis with the seven-day acute intraperitoneal LD50 value of above 6.0 × 109 cfu/ml and 30-day chronic oral LD50 of above 6.0 × 109 cfu/g diet. To our knowledge, this is the first report on the safety of R. azotoformans for potential application in Chinese mitten crabs.
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Affiliation(s)
- H Cao
- National Pathogen Collection Center for Aquatic Animals, Shanghai Ocean University, Shanghai 201306, China P.R
- Key Laboratory of Freshwater Fishery Germplasm Resources, Ministry of Agriculture and Rural Affairs of China, Shanghai 201306, China P.R
| | - S Zhang
- National Pathogen Collection Center for Aquatic Animals, Shanghai Ocean University, Shanghai 201306, China P.R
- Key Laboratory of Freshwater Fishery Germplasm Resources, Ministry of Agriculture and Rural Affairs of China, Shanghai 201306, China P.R
| | - X Zheng
- National Pathogen Collection Center for Aquatic Animals, Shanghai Ocean University, Shanghai 201306, China P.R
- Key Laboratory of Freshwater Fishery Germplasm Resources, Ministry of Agriculture and Rural Affairs of China, Shanghai 201306, China P.R
| | - L Xu
- Marine Science Research Institute of Shandong Province (National Oceanographic Center), Qingdao 266104, China P.R
- Shandong Key Laboratory of Disease Control in Mariculture, Qingdao 266104, China P.R
| | - J Diao
- Marine Science Research Institute of Shandong Province (National Oceanographic Center), Qingdao 266104, China P.R
- Shandong Key Laboratory of Disease Control in Mariculture, Qingdao 266104, China P.R
| | - Y Wang
- Marine Science Research Institute of Shandong Province (National Oceanographic Center), Qingdao 266104, China P.R
- Shandong Key Laboratory of Disease Control in Mariculture, Qingdao 266104, China P.R
| | - C Gai
- Marine Science Research Institute of Shandong Province (National Oceanographic Center), Qingdao 266104, China P.R
- Shandong Key Laboratory of Disease Control in Mariculture, Qingdao 266104, China P.R
| | - H Ye
- Marine Science Research Institute of Shandong Province (National Oceanographic Center), Qingdao 266104, China P.R
- Shandong Key Laboratory of Disease Control in Mariculture, Qingdao 266104, China P.R
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Li J, Chen Y, Wang X, He W, Liu C, Feng F, Zhang W, Cao H, Long Q, Gao F, Sun W. Homologous proteins SAPCD2X1 and SAPCD2 have significantly different carcinogenic capacities in human colorectal cancer cells based on structural prediction and functional verification. Cell Mol Biol (Noisy-le-grand) 2023; 69:8-15. [PMID: 38158695 DOI: 10.14715/cmb/2023.69.13.2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/02/2022] [Indexed: 01/03/2024]
Abstract
We discussed the expression and biological functions of the SAPCD2X1 protein in the HCT116 CRC cell line by bioinformatics analysis and prediction, and biological function verification. Spatial conformation models of SAPCD2X1 and SAPCD2 were predicted using the threading method, ensemble method, and several other protein structure prediction approaches. The conformational similarity between SAPCD2X1 and SAPCD2 was studied, and their functions were predicted. The biological experiments showed that SAPCD2X1 and SAPCD2 were overexpressed in CRC cells. SAPCD2X1-specific antibodies were prepared. The expressions of SAPCD2X1 and SAPCD2 were localized in cells using the immunofluorescence assay. The SAPCD2 and SAPCD2X1 overexpression models were validated using Western Blot and RT-qPCR. We successfully predicted the structures of the SAPCD2X1 and SAPCD2 proteins, and visualized them using the VDM software. It was predicted that the tertiary structure of SAPCD2X1 changed significantly compared with SAPCD2. Alteration of the biological functions of SAPCD2X1 was also predicted due to the changes in the spatial conformation of the protein. Anti-SAPCD2X1 antibody and SAPCD2X1-EGFP and SAPCD2-EGFP recombinant plasmids were established. The overexpression of the two proteins was induced in HCT116 cells using the recombinant plasmids, and verified by RT-qPCR and Western Blot. Meanwhile, the anti-SAPCD2X1 antibody was proved to have a high specificity. The immunofluorescence assay showed that SAPCD2X1 and SAPCD2 are mainly expressed in the cytoplasm. SAPCD2X1 and SAPCD2 exhibited significantly different biological functions in HCT116 cells. SAPCD2 is a carcinogenic protein, while SAPCD2X1 does not affect the proliferation, invasion, and migration of human CRC HCT116 cells.
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Affiliation(s)
- Jingchun Li
- Department of Central Laboratory, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Yuan Chen
- Department of Central Laboratory, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Xiaolong Wang
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Wenxi He
- Department of Central Laboratory, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Chunli Liu
- Department of Central Laboratory, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Feng Feng
- Department of Central Laboratory, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Wenwei Zhang
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Hongtao Cao
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Qixiong Long
- Department of Gastroenterology, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Fang Gao
- Department of Critical Care Medicine, Huadu District People's Hospital, Guangzhou 510800, China.
| | - Wei Sun
- Department of Central Laboratory, Huadu District People's Hospital, Guangzhou 510800, China.
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Wu Y, Cao H, Yang S, Liu C, Han Z. Progress of near-infrared-II fluorescence in precision diagnosis and treatment of colorectal cancer. Heliyon 2023; 9:e23209. [PMID: 38149207 PMCID: PMC10750080 DOI: 10.1016/j.heliyon.2023.e23209] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/18/2023] [Revised: 11/27/2023] [Accepted: 11/29/2023] [Indexed: 12/28/2023] Open
Abstract
Colorectal cancer is a malignant tumour with high incidence and mortality worldwide; therefore, improving the early diagnosis of colorectal cancer and implementing a targeted "individualized treatment" strategy is of great concern. NIR-II fluorescence imaging is a large-depth, high-resolution optical bioimaging tool. Around the NIR-II window, researchers have developed a variety of luminescent probes, imaging systems, and treatment methods with colorectal cancer targeting capabilities, which can be visualized and image-guided in clinical surgery. This article aims to overcome the difficulties in diagnosing and treating colorectal cancer. The present review summarizes the latest results on using NIR-II fluorescence for targeted colorectal cancer imaging, expounds on the application prospects of NIR-II optical imaging for colorectal cancer, and discusses the imaging-guided multifunctional diagnosis and treatment platforms.
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Affiliation(s)
- Yong Wu
- Third Hospital of Shanxi Medical University, Shanxi Bethune Hospital, Shanxi Academy of Medical Sciences, Tongji Shanxi Hospital, Taiyuan, 030032, China
| | - Hongtao Cao
- Third Hospital of Shanxi Medical University, Shanxi Bethune Hospital, Shanxi Academy of Medical Sciences, Tongji Shanxi Hospital, Taiyuan, 030032, China
| | - Shaoqing Yang
- Third Hospital of Shanxi Medical University, Shanxi Bethune Hospital, Shanxi Academy of Medical Sciences, Tongji Shanxi Hospital, Taiyuan, 030032, China
| | - Chaohui Liu
- Third Hospital of Shanxi Medical University, Shanxi Bethune Hospital, Shanxi Academy of Medical Sciences, Tongji Shanxi Hospital, Taiyuan, 030032, China
| | - Zhenguo Han
- Third Hospital of Shanxi Medical University, Shanxi Bethune Hospital, Shanxi Academy of Medical Sciences, Tongji Shanxi Hospital, Taiyuan, 030032, China
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Zhang KC, Meng XJ, Hu T, Luo D, Cao H, Lin QH, Zou HC. [Survey on the cognition of the "undetectable equals untransmittable" concept among HIV-infected men who have sex with men receiving antiviral treatment]. Zhonghua Liu Xing Bing Xue Za Zhi 2023; 44:1610-1615. [PMID: 37875449 DOI: 10.3760/cma.j.cn112338-20230424-00264] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Subscribe] [Scholar Register] [Indexed: 10/26/2023]
Abstract
Objective: To explore the cognition of the "undetectable equals untransmittable" ("U=U") concept and associated factors among HIV-infected men who have sex with men (MSM) receiving antiviral treatment (ART) in Shenzhen, and provide evidence for designing promotion and advocacy strategies for the "U=U" concept. Methods: We recruited HIV-infected MSM receiving ART using convenient sampling method combined with routine follow-up in Shenzhen through conducting observational survey. The sample size was estimated to be 475. A questionnaire was administered to collect socio-demographic characteristics, sexual behaviors, ART, viral load testing and the cognition towards "U=U" in HIV-infected MSM. Logistic regression was used to access factors associated with acceptance of "U=U". Results: A total of 490 HIV-infected MSM receiving ART were recruited. Of whom, 60.2% (295/490) were aware of "U=U" and 50.6% (248/490) accepted "U=U". Multiple logistic regression showed that participants who had an educational level of college or above (aOR=1.76,95%CI: 1.12-2.75) were more likely to accept "U=U". Those who had no local residency (aOR=0.51,95%CI: 0.29-0.92), had viral load >0 copies/ml in the last testing (aOR=0.61,95%CI: 0.38-0.98) and were unaware of "U=U" (aOR=0.13, 95%CI: 0.09-0.21), were less likely to accept "U=U". Conclusions: HIV-infected MSM receiving ART had a low cognition level of "U=U" in Shenzhen. Promotion and advocacy on this concept through healthcare workers should be enhanced in combination with routine follow-up in order to improve their ART adherence and outcome of treatment. Furthermore, developing related guidelines on "U=U" according to the characteristics of HIV-infected individuals is warranted to improve the normalization of promotion and advocacy on "U=U".
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Affiliation(s)
- K C Zhang
- Longhua District Centre for Disease Control and Prevention, Shenzhen 518109, China
| | - X J Meng
- Wuxi Prefectural Centre for Disease Control and Prevention, Wuxi 214023, China
| | - T Hu
- Longhua District Centre for Disease Control and Prevention, Shenzhen 518109, China
| | - D Luo
- School of Public Health (Shenzhen), Sun Yat-sen University, Shenzhen 518107, China
| | - H Cao
- Longhua District Centre for Disease Control and Prevention, Shenzhen 518109, China
| | - Q H Lin
- Longhua District Centre for Disease Control and Prevention, Shenzhen 518109, China
| | - H C Zou
- School of Public Health (Shenzhen), Sun Yat-sen University, Shenzhen 518107, China
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Qu C, He R, Hou W, Ye W, Cao H, Zhang H, Zhang N, Cheng Q, Zhang Q, Luo P. Global burden of neoplasms attributable to specific occupational carcinogens over 30 years: a population-based study. Public Health 2023; 223:145-155. [PMID: 37657137 DOI: 10.1016/j.puhe.2023.07.032] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/10/2023] [Revised: 07/16/2023] [Accepted: 07/25/2023] [Indexed: 09/03/2023]
Abstract
OBJECTIVES The study aimed to analyze the global burden of occupational neoplasms from various epidemiological perspectives. STUDY DESIGN In this cross-sectional study, secondary analyses were conducted to assess the burden of neoplasms attributable to occupational carcinogens and their distribution characteristics using data from GBD 2019 and the World Bank database. METHODS Based on the GBD 2019 and the World Bank database, we analyzed the global burden of occupational neoplasms including the age-period-cohort model, decomposition analysis, health inequality analysis, and panel model. All analyses were conducted in R (version 4.0.3) and Joinpoint (version 4.9.1). RESULTS The absolute number of neoplasms burden attributable to occupational carcinogens has continued to rise over 30 years. In 2019, occupational neoplasms caused 333,867 [95% uncertainty interval (UI): 263,491 to 404,641] mortalities and 6,964,775 (95% UI: 5,467,884 to 8,580,431) disability-adjusted life years (DALYs) globally. Greenland, Monaco, the Netherlands, and Andorra suffered the highest burden. The burden was higher in countries with a higher sociodemographic index. The age effect was prominent in the elderly, and the 1925 birth cohort had the highest cohort effect. Population growth was the most significant driver of the mortalities (89%) and DALYs (111%) change. Moreover, the proportion of urban population was significantly positively associated with the disease burden, while GDP per capita was negatively correlated with the disease burden. CONCLUSIONS The burden of occupational neoplasms was unevenly distributed across locations and populations. The need for rational allocation of healthcare resources was urgent.
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Affiliation(s)
- C Qu
- Department of Neurosurgery, Xiangya Hospital, Central South University, Changsha, Hunan, China; National Clinical Research Center for Geriatric Disorders, Xiangya Hospital, Central South University, Changsha, Hunan, China; XiangYa School of Medicine, Central South University, Changsha, Hunan, China
| | - R He
- Department of Neurosurgery, Xiangya Hospital, Central South University, Changsha, Hunan, China; National Clinical Research Center for Geriatric Disorders, Xiangya Hospital, Central South University, Changsha, Hunan, China; XiangYa School of Medicine, Central South University, Changsha, Hunan, China
| | - W Hou
- Department of Neurosurgery, Xiangya Hospital, Central South University, Changsha, Hunan, China; National Clinical Research Center for Geriatric Disorders, Xiangya Hospital, Central South University, Changsha, Hunan, China; XiangYa School of Medicine, Central South University, Changsha, Hunan, China
| | - W Ye
- Department of Neurosurgery, Xiangya Hospital, Central South University, Changsha, Hunan, China; National Clinical Research Center for Geriatric Disorders, Xiangya Hospital, Central South University, Changsha, Hunan, China
| | - H Cao
- Department of Psychiatry, Brain Hospital of Hunan Province (The Second People's Hospital of Hunan Province), Changsha, Hunan, China
| | - H Zhang
- Department of Neurosurgery, Xiangya Hospital, Central South University, Changsha, Hunan, China; Department of Neurosurgery, The Second Affiliated Hospital, Chongqing Medical University, Chongqing, China
| | - N Zhang
- College of Life Science and Technology, Huazhong University of Science and Technology, Wuhan, Hubei, China
| | - Q Cheng
- Department of Neurosurgery, Xiangya Hospital, Central South University, Changsha, Hunan, China; National Clinical Research Center for Geriatric Disorders, Xiangya Hospital, Central South University, Changsha, Hunan, China.
| | - Q Zhang
- Division of Gastroenterology and Hepatology, NHC Key Laboratory of Digestive Diseases, Shanghai Institute of Digestive Disease, Renji Hospital, School of Medicine, Shanghai Jiao Tong University, Shanghai, China.
| | - P Luo
- Department of Oncology, Zhujiang Hospital, Southern Medical University, Guangzhou, Guangdong, China.
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Bo Y, Hou P, Wan J, Cao H, Liu Y, Xie L, Guldi DM. One-Pot Synthesis and Excited-State Dynamics of Null Exciton-Coupled Diketopyrrolopyrroles Oligo-Grids. Adv Mater 2023; 35:e2302664. [PMID: 37289569 DOI: 10.1002/adma.202302664] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/22/2023] [Revised: 06/02/2023] [Indexed: 06/10/2023]
Abstract
Exciton coupling in molecular aggregates plays a vital role in impacting and fine-tuning optoelectronic materials and their efficiencies in devices. A versatile platform to decipher aggregation-property relationships is built around multichromophoric architectures. Here, a series of cyclic diketopyrrolopyrrole (DPP) oligomers featuring nanoscale gridarene structures and rigid bifluorenyl spacers are designed and synthesized via one-pot Friedel-Crafts reaction. DPP dimer [2]Grid and trimer [3]Grid, which are cyclic rigid nanoarchitectures of rather different sizes, are further characterized via steady-state and time-resolved absorption and fluorescence spectroscopies. They exhibit monomer-like spectroscopic signatures in the steady-state measurements, from which null exciton couplings are derived. Moreover, in an apolar solvent, high fluorescence quantum yields and excited-state dynamics that resembled DPP monomer are gathered. In a polar solvent, the localized singlet excited state on a single DPP dissociates into the adjacent null coupling DPP with charge transfer characteristics. This pathway facilitates the evolution of the symmetry-broken charge-separated state (SB-CS). Notable is the fact that the SB-CS of [2]Grid is, on one hand, in equilibrium with the singlet excited state and promotes, on the other hand, the formation of the triplet excited state with a yield of 32% via charge recombination.
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Affiliation(s)
- Yifan Bo
- Department of Chemistry and Pharmacy, Interdisciplinary Center for Molecular Materials (ICMM), Friedrich-Alexander-Universität Erlangen-Nürnberg, Egerlandstr. 3, 91058, Erlangen, Germany
| | - Pengfei Hou
- Key Laboratory for Organic Electronics and Information Displays, Institute of Advanced Materials, Center for Molecular Systems and Organic Devices (CMSOD), Nanjing University of Posts and Telecommunications, 9 Wenyuan Road, Nanjing, 210023, China
| | - Jun Wan
- Key Laboratory for Organic Electronics and Information Displays, Institute of Advanced Materials, Center for Molecular Systems and Organic Devices (CMSOD), Nanjing University of Posts and Telecommunications, 9 Wenyuan Road, Nanjing, 210023, China
| | - Hongtao Cao
- Key Laboratory for Organic Electronics and Information Displays, Institute of Advanced Materials, Center for Molecular Systems and Organic Devices (CMSOD), Nanjing University of Posts and Telecommunications, 9 Wenyuan Road, Nanjing, 210023, China
| | - Yuyu Liu
- College of Electrical Engineering, Nanjing Vocational University of Industry Technology, 1 Yangshan North Road, Nanjing, 210023, China
| | - Linghai Xie
- Key Laboratory for Organic Electronics and Information Displays, Institute of Advanced Materials, Center for Molecular Systems and Organic Devices (CMSOD), Nanjing University of Posts and Telecommunications, 9 Wenyuan Road, Nanjing, 210023, China
| | - Dirk M Guldi
- Department of Chemistry and Pharmacy, Interdisciplinary Center for Molecular Materials (ICMM), Friedrich-Alexander-Universität Erlangen-Nürnberg, Egerlandstr. 3, 91058, Erlangen, Germany
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Zhang Q, Liu N, Li Y, Guo JY, Huang QS, Cao H, Li Y, Yin ZQ, Liu MY, Wang ZY, Qi SJ, Fang MX. Effect of mechanical ventilation guided by transpulmonary pressure in acute respiratory distress syndrome patients: a systematic review and meta-analysis of randomized control trials. Eur Rev Med Pharmacol Sci 2023; 27:7020-7030. [PMID: 37606111 DOI: 10.26355/eurrev_202308_33274] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 08/23/2023]
Abstract
OBJECTIVE This study aimed to investigate the effect of mechanical ventilation guided by transpulmonary pressure in patients diagnosed with acute respiratory distress syndrome (ARDS). MATERIALS AND METHODS Randomized control trials of ARDS patients that received mechanical ventilation guided by transpulmonary pressure vs. mechanical ventilation guided by traditional lung protective ventilation strategies in adults were retrieved by two reviewers independently from PubMed, EMBASE, The Cochrane Library, The China National Knowledge Infrastructure, and WanFang database before October 2022. The protocol has been registered on PROSPERO (CRD42022307816). The primary outcome was mortality. The secondary outcomes included mechanical ventilation days, oxygenation function and ventilation parameters, hemodynamics, and cytokines level. RESULTS Thirteen articles (819 patients) were finally included through our search strategy. The total mortality (RR, 0.68; 95% CI, 0.54-0.85; p = 0.0006) and mechanical ventilation days (MD, -2.77; 95% CI, -4.60 - -0.94; p = 0.003) reduced when compared with the control group. Patients in the transpulmonary pressure group had higher oxygen index (MD, 40.74; 95% CI 9.81-71.68, p = 0.010) and lung compliance (MD, 7.98; 95% CI 4.55-11.41, p < 0.00001). Positive end-expiratory pressure (PEEP) was higher in the transpulmonary pressure group (MD, 5.47; 95% CI, 3.59 - 7.35; p < 0.00001). The Interlukin-6 (IL-6) level in the control group decreased obviously compared with that in the transpulmonary pressure group (SMD, -2.03; 95% CI, -3.50 - -0.56; p = 0.007). CONCLUSIONS Mechanical ventilation guided by transpulmonary pressure tended to have a beneficial prognosis on ARDS patients. Oxygenation and lung mechanics parameters were also improved. The clinical effect of mechanical ventilation directed by transpulmonary pressure was superior to the traditional lung protective ventilation strategies in ARDS patients.
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Affiliation(s)
- Q Zhang
- Department of Critical Care Medicine, The Third Hospital of Hebei Medical University, Hebei, China.
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20
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Gao K, Wang Y, Cao H, Jia J. [Efficacy of machine learning models versus Cox regression model for predicting prognosis of esophagogastric junction adenocarcinoma]. Nan Fang Yi Ke Da Xue Xue Bao 2023; 43:952-963. [PMID: 37439167 DOI: 10.12122/j.issn.1673-4254.2023.06.10] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 07/14/2023]
Abstract
OBJECTIVE To compare the performance of machine learning models and traditional Cox regression model in predicting postoperative outcomes of patients with esophagogastric junction adenocarcinoma (AEG). METHODS This study was conducted among 203 AEG patients with complete clinical and follow-up data, who were treated in our hospital between September, 2015 and October, 2020. The clinicopathological data of the patients were processed for analysis using R language package and divided into training and validation datasets at the ratio of 3:1. The Cox proportional hazards regression model and 4 machine learning models were constructed for analyzing the datasets. ROC curves, calibration curves and clinical decision curves (DCA) were plotted. Internal validation of the machine learning models was performed to assess their predictive efficacy. The predictive performance of each model was evaluated by calculating the area under the curve (AUC), and the model fitting was assessed using the calibration curve. RESULTS For predicting 3-year survival based on the validation dataset, the AUC was 0.870 for Cox proportional hazard regression model, 0.901 for eXtreme Gradient Boosting (XGBoost), 0.791 for random forest, 0.832 for support vector machine, and 0.725 for multilayer perceptron; For predicting 5-year survival, the AUCs of these models were 0.915, 0.916, 0.758, 0.905, and 0.737, respectively. For internal validation, the AUCs of the 4 machine learning models decreased in the order of XGBoost (0.818), random forest (0.758), support vector machine (0.0.804), and multilayer perceptron (0.745). CONCLUSION The machine learning models show better predictive efficacy for survival outcomes of patients with AEG than Cox proportional hazard regression model, especially when proportional odds assumption or linear regression models are not applicable. XGBoost models have better performance than the other machine learning models, and the multi-layer perception model may have poor fitting results for a limited data volume.
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Affiliation(s)
- K Gao
- Department of Surgical Oncology, First Affiliated Hospital of Bengbu Medical College, Bengbu 233000, China
| | - Y Wang
- Department of Surgical Oncology, First Affiliated Hospital of Bengbu Medical College, Bengbu 233000, China
| | - H Cao
- Department of Surgical Oncology, First Affiliated Hospital of Bengbu Medical College, Bengbu 233000, China
| | - J Jia
- Department of Surgical Oncology, First Affiliated Hospital of Bengbu Medical College, Bengbu 233000, China
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Zhang R, Lin T, Peng S, Bi J, Zhang S, Su G, Sun J, Gao J, Cao H, Zhang Q, Gu L, Cao Y. Flexible but Refractory Single-Crystalline Hyperbolic Metamaterials. Nano Lett 2023; 23:3879-3886. [PMID: 37115190 DOI: 10.1021/acs.nanolett.3c00512] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/11/2023]
Abstract
The fabrication of flexible single-crystalline plasmonic or photonic components in a scalable way is fundamentally important to flexible electronic and photonic devices with high speed, high energy efficiency, and high reliability. However, it remains a challenge. Here, we have successfully synthesized flexible single-crystalline optical hyperbolic metamaterials by directly depositing refractory nitride superlattices on flexible fluorophlogopite-mica substrates with magnetron sputtering. Interestingly, these flexible hyperbolic metamaterials show dual-band hyperbolic dispersion of dielectric constants with small dielectric losses and high figures of merit in the visible to near-infrared ranges. More importantly, the optical properties of these nitride-based flexible hyperbolic metamaterials show remarkable stability during 1000 °C heating or after being bent 1000 times. Therefore, the strategy developed in this work offers an easy and scalable route for fabricating flexible, high-performance, and refractory plasmonic or photonic components, which can significantly expand the applications of current electronic and photonic devices.
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Affiliation(s)
- Ruyi Zhang
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Ting Lin
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Shaoqin Peng
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Jiachang Bi
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Shunda Zhang
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Guanhua Su
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Jie Sun
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Junhua Gao
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Hongtao Cao
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Qinghua Zhang
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Lin Gu
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Yanwei Cao
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
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22
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Liang L, Zhang H, Li T, Li W, Gao J, Zhang H, Guo M, Gao S, He Z, Liu F, Ning C, Cao H, Yuan G, Liu C. Addressing the Conflict between Mobility and Stability in Oxide Thin-film Transistors. Adv Sci (Weinh) 2023; 10:e2300373. [PMID: 36935362 DOI: 10.1002/advs.202300373] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/17/2023] [Revised: 02/28/2023] [Indexed: 05/18/2023]
Abstract
Amorphous oxide semiconductor thin-film transistors (AOS TFTs) are ever-increasingly utilized in displays. However, to bring high mobility and excellent stability together is a daunting challenge. Here, the carrier transport/relaxation bilayer stacked AOS TFTs are investigated to solve the mobility-stability conflict. The charge transport layer (CTL) is made of amorphous In-rich InSnZnO, which favors big average effective coordination number for all cations and more edge-shared structures for better charge transport. Praseodymium-doped InSnZnO is used as the charge relaxation layer (CRL), which substantially shortens the photoelectron lifetime as revealed by femtosecond transient absorption spectroscopy. The CTL and CRL with the thickness suitable for industrial production respectively afford minute potential barrier fluctuation for charge transport and fast relaxation for photo-generated carriers, resulting in transistors with an ultrahigh mobility (75.5 cm2 V-1 s-1 ) and small negative-bias-illumination-stress/positive-bias-temperature-stress voltage shifts (-1.64/0.76 V). The design concept provides a promising route to address the mobility-stability conflict for high-end displays.
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Affiliation(s)
- Lingyan Liang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Hengbo Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Ting Li
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Wanfa Li
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Junhua Gao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Hongliang Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Min Guo
- State Key Lab of Opto-Electronic Materials and Technologies, School of Electronics and Information Technology, Sun Yat-Sen University, Guangzhou, 510275, P. R. China
| | - Shangpeng Gao
- Department of Materials Science, Fudan University, Shanghai, 200433, P. R. China
| | - Zirui He
- Department of Materials Science, Fudan University, Shanghai, 200433, P. R. China
| | - Fengjuan Liu
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo, 315201, P. R. China
| | - Ce Ning
- BOE Technology Group Co. Ltd., Beijing, 100176, P. R. China
| | - Hongtao Cao
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing, 100049, P. R. China
| | - Guangcai Yuan
- BOE Technology Group Co. Ltd., Beijing, 100176, P. R. China
| | - Chuan Liu
- State Key Lab of Opto-Electronic Materials and Technologies, School of Electronics and Information Technology, Sun Yat-Sen University, Guangzhou, 510275, P. R. China
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Zhou Y, Xia T, Du M, Cao H, Zheng Q, Yang J, Yan Z. The strategy to track and combat the deep sternal wound infection caused by Mycobacterium farcinogenes. J Hosp Infect 2023:S0195-6701(23)00102-0. [PMID: 37001604 DOI: 10.1016/j.jhin.2023.03.016] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/16/2023] [Accepted: 03/22/2023] [Indexed: 03/31/2023]
Affiliation(s)
- Y Zhou
- Department of Laboratory Medicine, Second Medical Centre of PLA General Hospital, Beijing, People's Republic of China
| | - T Xia
- Department of Disease Prevention and Control, Hainan Hospital of PLA General Hospital, Sanya, Hainan, People's Republic of China
| | - M Du
- Department of Disease Prevention and Control, First Medical Centre of PLA General Hospital, Beijing, People's Republic of China
| | - H Cao
- Department of Laboratory Medicine, Second Medical Centre of PLA General Hospital, Beijing, People's Republic of China
| | - Q Zheng
- Department of Laboratory Medicine, Second Medical Centre of PLA General Hospital, Beijing, People's Republic of China
| | - J Yang
- Department of Disease Prevention and Control, Hainan Hospital of PLA General Hospital, Sanya, Hainan, People's Republic of China
| | - Z Yan
- Department of Disease Prevention and Control, Hainan Hospital of PLA General Hospital, Sanya, Hainan, People's Republic of China; Department of Disease Prevention and Control, Second Medical Centre of PLA General Hospital, Beijing, People's Republic of China.
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Cao H, Zhang ZZ, Zhu CC. [Influence of postoperative complications on prognosis of gastric cancer-The manifestation of gastric surgeon's skill, responsibility and empathy]. Zhonghua Wei Chang Wai Ke Za Zhi 2023; 26:126-131. [PMID: 36797557 DOI: 10.3760/cma.j.cn441530-20221102-00447] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Subscribe] [Scholar Register] [Indexed: 02/18/2023]
Abstract
Radical gastrectomy combined with perioperative comprehensive treatment is the main curable strategy for gastric cancer patients, and postoperative complications are the issue that gastric surgeons have to face. Complications not only affect the short-term postoperative recovery, but also facilitate tumor recurrence or metastasis, thus resulting in poor prognosis. Therefore, unifying the diagnostic criteria for postoperative complications, bringing the surgeons' attention to complications, and understanding the potential mechanism of complications undermining long-term survival, will be helpful to the future improvement of the clinical diagnosis and treatment as well as prognosis for gastric cancer patients in China. Meanwhile, surgeons should constantly hone their operative skills, improve their sense of responsibility and empathy, and administer individualized perioperative management based on patients' general conditions, so as to minimize the occurrence of postoperative complications and their influence on prognosis.
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Affiliation(s)
- H Cao
- Department of Gastrointestinal Surgery, Ren Ji Hospital,Shanghai Jiao Tong University School of Medicine, Shanghai 200127, China
| | - Z Z Zhang
- Department of Gastrointestinal Surgery, Ren Ji Hospital,Shanghai Jiao Tong University School of Medicine, Shanghai 200127, China
| | - C C Zhu
- Department of Gastrointestinal Surgery, Ren Ji Hospital,Shanghai Jiao Tong University School of Medicine, Shanghai 200127, China
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Chen X, Wang K, Chu D, Zhu Y, Zhang W, Cao H, Xie W, Lu C, Li X. [Forsythiaside B inhibits cerebral ischemia/reperfusion-induced oxidative stress injury in mice via the AMPK/DAF-16/FOXO3 pathway]. Nan Fang Yi Ke Da Xue Xue Bao 2023; 43:199-205. [PMID: 36946038 PMCID: PMC10034537 DOI: 10.12122/j.issn.1673-4254.2023.02.06] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 03/23/2023]
Abstract
OBJECTIVE To study the protective effect of forsythiaside B (FB) against cerebral oxidative stress injury induced by cerebral ischemia/reperfusion (I/R) in mice and explore the underlying mechanism. METHODS Ninety C57BL/6 mice were randomized into sham-operated group, middle cerebral artery occlusion (MCAO) model group, and low-, medium and highdose (10, 20, and 40 mg/kg, respectively) FB groups. The expression levels of MDA, ROS, PCO, 8-OHdG, SOD, GSTα4, CAT and GPx in the brain tissue of the mice were detected using commercial kits, and those of AMPK, P-AMPK, DAF-16, FOXO3 and P-FOXO3 were detected with Western blotting. Compound C (CC), an AMPK inhibitor, was used to verify the role of the AMPK pathway in mediating the therapeutic effect of FB. In another 36 C57BL/6 mice randomized into 4 sham-operated group, MCAO model group, FB (40 mg/kg) treatment group, FB+CC (10 mg/kg) treatment group, TTC staining was used to examine the volume of cerebral infarcts, and the levels of ROS and SOD in the brain were detected; the changes in the protein expressions of AMPK, P-AMPK, DAF-16, FOXO3 and P-FOXO3 in the brain tissue were detected using Western blotting. RESULTS In mice with cerebral IR injury, treatment with FB significantly reduced the levels of ROS, MDA, PCO and 8-OHdG, increased the activities of antioxidant enzymes SOD, GSTα4, CAT and GPx, and enhanced phosphorylation of AMPK and FOXO3 and DAF-16 protein expression in the brain tissue (P < 0.01). Compared with FB treatment alone, the combined treatment with FB and CC significantly reduced phosphorylation of AMPK and FOXO3, lowered expression of DAF-16 and SOD activity, and increased cerebral infarction volume and ROS level in the brain tissue of the mice (P < 0.01). CONCLUSION FB inhibits oxidative stress injury caused by cerebral I/R in mice possibly by enhancing AMPK phosphorylation, promoting the downstream DAF-16 protein expression and FOXO3 phosphorylation, increasing the expression of antioxidant enzymes, and reducing ROS level in the brain tissue.
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Affiliation(s)
- X Chen
- Department of Critical Care Medicine, Hanbin District Third People's Hospital, Ankang 725000, China
| | - K Wang
- Department of Critical Care Medicine, Hanbin District Third People's Hospital, Ankang 725000, China
| | - D Chu
- Department of Critical Care Medicine, Hanbin District Third People's Hospital, Ankang 725000, China
| | - Y Zhu
- Department of Critical Care Medicine, Hanbin District Third People's Hospital, Ankang 725000, China
| | - W Zhang
- Department of Critical Care Medicine, Hanbin District Third People's Hospital, Ankang 725000, China
| | - H Cao
- Department of Critical Care Medicine, Hanbin District Third People's Hospital, Ankang 725000, China
| | - W Xie
- Department of Neurosurgery, Xijing Hospital, Air Force Medical University, Xi'an 710032, China
| | - C Lu
- Department of Neurosurgery, Xijing Hospital, Air Force Medical University, Xi'an 710032, China
| | - X Li
- Department of Neurosurgery, Xijing Hospital, Air Force Medical University, Xi'an 710032, China
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Ma W, Li Z, Cao H, Liang L, Lu H, Liu Y, Song Y. Modulating the nonlinear absorption response of SnO x thin films via phase engineering. Opt Express 2023; 31:6252-6261. [PMID: 36823886 DOI: 10.1364/oe.484846] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/03/2023] [Accepted: 01/23/2023] [Indexed: 06/18/2023]
Abstract
Phase (composition) is known to play a key role in determining the electronic and optical properties of amorphous oxide semiconductors. In this work, modulating the ultrafast nonlinear optical (NLO) response of SnO2 and SnO thin films by tuning oxygen partial pressure during film sputtering is explored. Femtosecond Z-scan results demonstrate that intermediate phases have no profound impact on the two-photon absorption (TPA) response of SnO2 and SnO films. Interestingly, the magnitude of the effective nonlinear absorption coefficient (βeff) of both intermediate SnO2-x and SnOx are enhanced after the change of Sn2+/Sn4+ composition ratio, as measured by picosecond Z-scan technique. Femtosecond degenerate pump-probe measurements show that intermediate phases accelerate the carrier trapping and improve the defect-related carrier absorption in SnOx (SnO-rich) film, while intermediate phase suppress the TPA response of SnO2-x (SnO2-rich) films, therefore carrier-induced absorption dominates the NLO behavior of SnO2-x film on picosecond regime. Our results indicate a simple and effective way to modulate the NLO response of transparent conductive oxide SnO2 and SnO.
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Lai Y, Lee Y, Cao H, Zhang H, Chen B. Extraction of heterocyclic amines and polycyclic aromatic hydrocarbons from pork jerky and the effect of flavoring on formation and inhibition. Food Chem 2023; 402:134291. [DOI: 10.1016/j.foodchem.2022.134291] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/08/2022] [Revised: 09/12/2022] [Accepted: 09/13/2022] [Indexed: 10/14/2022]
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Fei Z, Pan B, Pei R, Ye S, Wang Z, Ma L, Zhang R, Li C, Du X, Cao H. Neuroprotective Effects of IVIG against Alzheimer' s Disease via Regulation of Antigen Processing and Presentation by MHC Class I Molecules in 3xTg-AD Mice. J Prev Alzheimers Dis 2023; 10:581-594. [PMID: 37357300 DOI: 10.14283/jpad.2023.56] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 06/27/2023]
Abstract
BACKGROUND The results of clinical trials for Alzheimer's disease (AD) patients treated with Intravenous immunoglobulin (IVIG) revealed inconsistency in efficacy. OBJECTIVE To explore the neuroprotective effects and possible mechanisms of different IVIG in 3xTg-AD mice. METHODS 3-month-old 3xTg-AD mice were administered intraperitoneally with different IVIG (A/B/C) for 3 months and then the therapeutic effects were observed and tested at 9 months of age. The bioavailability of IVIG and Aβ40/42 concentrations in parietotemporal cortex was measured by ELISA. Behavioral tests were performed to examine cognitive functions. Immunohistochemistry was utilized to examine the deposition of Aβ, the phosphorylation of tau, the levels of GFAP and Iba-1 in the hippocampus. Proteomics, Luminex assay and parallel reaction monitoring were performed to identify and verify the proteins that showed a marked change in the hippocampus. RESULTS IVIG-C was more effective than IVIG-A and IVIG-B in counteracting cognitive deficits, ameliorating Aβ deposits and tau phosphorylation, attenuating the activation of microglia and astrocytes in the hippocampus and inhibiting the secretion of pro-inflammatory factors. IVIG-C affected innate immunity and suppressed the activation of antigen processing and presentation by MHC class I molecule (APP-MHC-I). CONCLUSION The efficacy of different IVIG on AD was significantly different, and only IVIG-C has been confirmed to possess significant neuroprotective effects, which are related to the inhibition of APP-MHC-I. IVIG may be a potential therapeutic for AD but further research is needed to evaluate the functional of IVIG before clinical trials of AD treatment.
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Affiliation(s)
- Z Fei
- Xi Du and Haijun Cao , Institute of Blood Transfusion, Chinese Academy of Medical Sciences and Peking Union Medical College, Chengdu 610052, China, ; . Tel: 86-28-61648527
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Zhao B, Qin C, Li Z, Wang Y, Li T, Cao H, Yang X, Li T, Wang W. Multidrug resistance genes screening of pancreatic ductal adenocarcinoma based on sensitivity profile to chemotherapeutic drugs. Cancer Cell Int 2022; 22:374. [PMID: 36457017 PMCID: PMC9714099 DOI: 10.1186/s12935-022-02785-7] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/22/2022] [Accepted: 11/09/2022] [Indexed: 12/03/2022] Open
Abstract
BACKGROUNDS Pancreatic ductal adenocarcinoma (PDAC) is one of the most lethal cancer types and chemotherapeutic drug resistance is a stumbling block in improving the overall survival of PDAC patients. The nature of specific drug resistant subpopulation within pancreatic ductal adenocarcinoma is believed to be partly attributed to epithelial-mesenchymal transition (EMT) and cell stemness. Various PDAC cell lines show various degrees of resistance to chemotherapeutic agents including gemcitabine (GEM) and 5-fluorouracil (5-FU). In-depth understanding of drug resistance mechanisms and profile heterogeneities could lead to the development of novel and precise therapeutic strategies for addressing the chemo-resistant dilemma in PDAC patients. METHODS Cytotoxicity assays were performed by CCK8 in ten common PDAC cell lines including AsPC-1, BxPC-3, CAPAN-1, CFPAC, HPAFII, MIA PaCa-2, PANC-1, Patu-8988, SW1990 and T3M4. RNA-seq data of the ten cell lines were downloaded from Cancer Cell Line Encyclopedia (CCLE) database and subsequently analyzed for differentially expressed genes (DEGs). Based on first-line chemotherapy regimens of PDAC, DEGs between resistant and sensitive cell lines were validated by qRT-PCR. Enriched pathways of differentially expressed genes between the resistant and sensitive cell lines were acquired by Metascape database. RESULTS We found that the top two toxic drugs for PDAC cell lines were paclitaxel (PTX) and GEM. Among the ten PDAC cell lines, SW1990 was the most resistant PDAC cell line with the highest IC50 levels for three drugs, while MIA PaCa-2 and BxPC-3 were the most sensitive PDAC cell lines. Differential expression analysis revealed the highest number of DEGs associated with cisplatin (CIS) sensitivity up to 642 genes, of which 181 genes were upregulated and 461 genes were downregulated in CIS-resistant cell lines. The least number of DEGs are associated with GEM sensitivity, of which 37 genes were highly expressed in GEM-resistant PDAC cell lines and 25 genes were lowly expressed. Enrichment analysis of the DEGs revealed that pathways associated with drug resistance were mainly extracellular matrix and cell-cell junction related pathways. CONCLUSIONS PDAC cell lines showed diverse sensitivities to commonly used chemotherapeutic agents, which was caused by differential gene expression between the resistant and sensitive cell lines. The heterogeneity and its associated genes were enriched in extracellular matrix and cell-cell junction related pathways. Our study first portrayed the sensitivity profile to chemotherapeutic drugs of PDAC, which would benefit the chemoresistance mechanism study by reemphasizing the vital role of extracellular matrix and cell-cell junction related pathways and helping the selection of suitable PDAC cell lines.
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Affiliation(s)
- Bangbo Zhao
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Cheng Qin
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Zeru Li
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Yuanyang Wang
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Tianhao Li
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Hongtao Cao
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Xiaoying Yang
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Tianyu Li
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
| | - Weibin Wang
- grid.506261.60000 0001 0706 7839Department of General Surgery, State Key Laboratory of Complex Severe and Rare Diseases, Peking Union Medical College Hospital, Chinese Academy of Medical Sciences and Peking Union Medical College, Beijing, 100730 China
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Cao H, Jung TP, Chen Y, Mei J, Li A, Xu M, Ming D. [Research advances in non-invasive brain-computer interface control strategies]. Sheng Wu Yi Xue Gong Cheng Xue Za Zhi 2022; 39:1033-1040. [PMID: 36310493 DOI: 10.7507/1001-5515.202205013] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 06/16/2023]
Abstract
Brain-computer interface (BCI) can establish a direct communications pathway between the human brain and the external devices, which is independent of peripheral nerves and muscles. Compared with invasive BCI, non-invasive BCI has the advantages of low cost, low risk, and ease of operation. In recent years, using non-invasive BCI technology to control devices has gradually evolved into a new type of human-computer interaction manner. Moreover, the control strategy for BCI is an essential component of this manner. First, this study introduced how the brain control techniques were developed and classified. Second, the basic characteristics of direct and shared control strategies were thoroughly explained. And then the benefits and drawbacks of these two strategies were compared and further analyzed. Finally, the development direction and application prospects for non-invasive brain control strategies were suggested.
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Affiliation(s)
- Hongtao Cao
- Institute of Medical Engineering and Translational Medicine, Tianjin University, Tianjin 300072, P. R. China
| | - Tzyy-Ping Jung
- Institute of Medical Engineering and Translational Medicine, Tianjin University, Tianjin 300072, P. R. China
- School of Precision Instruments and Optoelectronic Engineering, Tianjin University Tianjin 300072, P. R. China
- University of California, Swartz Center for Computational Sciences, California 92093, USA
| | - Yuanfang Chen
- Beijing Institute of Machinery and Equipment, Beijing 100854, P. R. China
| | - Jie Mei
- School of Precision Instruments and Optoelectronic Engineering, Tianjin University Tianjin 300072, P. R. China
| | - Ang Li
- School of Precision Instruments and Optoelectronic Engineering, Tianjin University Tianjin 300072, P. R. China
| | - Minpeng Xu
- Institute of Medical Engineering and Translational Medicine, Tianjin University, Tianjin 300072, P. R. China
- School of Precision Instruments and Optoelectronic Engineering, Tianjin University Tianjin 300072, P. R. China
| | - Dong Ming
- Institute of Medical Engineering and Translational Medicine, Tianjin University, Tianjin 300072, P. R. China
- School of Precision Instruments and Optoelectronic Engineering, Tianjin University Tianjin 300072, P. R. China
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Wang Y, Xiao J, Cao H, Xing J, Cong H, Shen Y, Yu B. Preparation and modification of PS-PMMA microspheres and their application in high performance liquid chromatography. Anal Methods 2022; 14:3999-4007. [PMID: 36193655 DOI: 10.1039/d2ay01425d] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/16/2023]
Abstract
Polymer microspheres have been widely used as a stationary phase for liquid chromatography. In this work, we prepared and synthesized polystyrene-methyl methacrylate (PS-PMMA) microspheres, modified them, characterized the microspheres to have good chromatographic properties, and then used them as a high-performance liquid chromatography (HPLC) stationary phase to explore their applications. First, the PS-PMMA microspheres were hydrolyzed, and the separation of benzene homologues/alkaloids was explored. Then, on the basis of hydrolysis, diazo resin (DR) was used as a coupling agent to further modify the surface of the microspheres with amphoteric glycopeptide vancomycin. The modified microspheres were used as a HPLC stationary phase to explore the application of the stationary phase in the separation of chiral drugs. This work is important to broaden the application of functional chiral columns for antibiotics and to expand the application of PS-PMMA microspheres in HPLC.
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Affiliation(s)
- Yu Wang
- Institute of Biomedical Materials and Engineering, College of Materials Science and Engineering, Shandong University of Technology, Zibo 255000, China.
- State Key Laboratory of Bio-Fibers and Eco-Textiles, College of Chemistry and Chemical Engineering, Qingdao University, Qingdao 266071, China.
| | - Jingyuan Xiao
- Institute of Biomedical Materials and Engineering, College of Materials Science and Engineering, Shandong University of Technology, Zibo 255000, China.
| | - Hongtao Cao
- Institute of Biomedical Materials and Engineering, College of Materials Science and Engineering, Shandong University of Technology, Zibo 255000, China.
| | - Jie Xing
- Institute of Biomedical Materials and Engineering, College of Materials Science and Engineering, Shandong University of Technology, Zibo 255000, China.
| | - Hailin Cong
- Institute of Biomedical Materials and Engineering, College of Materials Science and Engineering, Shandong University of Technology, Zibo 255000, China.
- State Key Laboratory of Bio-Fibers and Eco-Textiles, College of Chemistry and Chemical Engineering, Qingdao University, Qingdao 266071, China.
| | - Youqing Shen
- State Key Laboratory of Bio-Fibers and Eco-Textiles, College of Chemistry and Chemical Engineering, Qingdao University, Qingdao 266071, China.
| | - Bing Yu
- State Key Laboratory of Bio-Fibers and Eco-Textiles, College of Chemistry and Chemical Engineering, Qingdao University, Qingdao 266071, China.
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Li Z, Wu H, Cao H, Liang L, Han Y, Yang J, Song Y, Burda C. Improved Ultrafast Carrier Relaxation and Charge Transfer Dynamics in CuI Films and Their Heterojunctions via Sn Doping. J Phys Chem Lett 2022; 13:9072-9078. [PMID: 36154177 DOI: 10.1021/acs.jpclett.2c02354] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 06/16/2023]
Abstract
CuI is one of the promising hole transport materials for perovskite solar cells. However, its tendency to form defects is currently limiting its use for device applications. Here, we report the successful improvement of CuI through Sn doping and the direct measurement of the carrier relaxation and interfacial charge-transfer processes in Sn-doped CuI films and their heterostructures. Femtosecond-transient absorption (fs-TA) measurements reveal that Sn doping effectively passivates the trap states within the bandgap of CuI. The I-V characteristics of heterostructures demonstrate drastic improvement in transport characteristics upon Sn doping. Fs-TA measurements further confirm that the CuSnI/ZnO heterojunction has a type-II configuration with ultrafast charge transfer (<280 fs). The charge transfer time of a CuI/ZnO heterostructure is ∼2.8 times slower than that of the CuSnI/ZnO heterostructure, indicating that Sn doping suppresses the interfacial states that retard the charge transfer. These results elucidate the effect of Sn doping on the performance of CuI-based heterostructures.
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Affiliation(s)
- Zhongguo Li
- School of Electronic and Information Engineering, Changshu Institute of Technology, Changshu 215500, China
| | - Haijuan Wu
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Lingyan Liang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Yanbing Han
- Department of Physics, Harbin Institute of Technology, Harbin 150001, China
| | - Junyi Yang
- School of Physical Science and Technology, Soochow University, Suzhou 215006, China
| | - Yinglin Song
- Department of Physics, Harbin Institute of Technology, Harbin 150001, China
| | - Clemens Burda
- Department of Chemistry, College of Arts and Sciences, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, United States
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Ren J, Sun Y, Dai B, Song W, Tan T, Guo L, Cao H, Wu Y, Hu W, Wang Z, Haiping D. Association between Ca2+ Signaling Pathway-Related Gene Polymorphism and Age-Related Hearing Loss in Qingdao Chinese Elderly. RUSS J GENET+ 2022. [DOI: 10.1134/s1022795422100076] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Zhang YF, Li XB, Hong YG, Li XM, Liang WM, Zheng ZX, Yang GY, Wen YY, Cao H, Wu WL, Su WZ. 1252P Update results of anlotinib combined with nab-paclitaxel and cisplatin as neoadjuvant treatment for esophageal squamous cell carcinoma (ESCC): A single-arm, open-label phase Ⅱ clinical trial. Ann Oncol 2022. [DOI: 10.1016/j.annonc.2022.07.1370] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022] Open
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Pei Y, Liang L, Wang X, Wang Z, Zhang H, Ren J, Cao H. Low-Temperature-Crystallized Ga 2O 3 Thin Films and Their TFT-Type Solar-Blind Photodetectors. J Phys Chem Lett 2022; 13:7243-7251. [PMID: 35913457 DOI: 10.1021/acs.jpclett.2c01852] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 06/15/2023]
Abstract
Crystalline Ga2O3 (c-Ga2O3) is a promising candidate for next-generation solar-blind photodetectors (SBPDs) but is suffering from high processing temperatures. Herein, seed-induced engineering is proposed via adopting Zn as an induced metal for crystallizing Ga2O3, lowering the processing temperature by 200 °C. After annealing, the Zn/Ga2O3 consists of an inner Ga2O3 layer of a monoclinic crystalline phase, top ZnO crystals coming from Zn oxidation, and a thin corundum Ga2O3 layer between them, which implies a "seed-induced" crystallization mechanism besides the nonequilibrium chaotic state caused by the traditional electron transfer one. As a result, the tailored c-Ga2O3 thin-film transistor-type SBPD with enhanced packing density and finite oxygen deficiency demonstrates a satisfactory responsivity of 8.6 A/W and also an ultrahigh UVC/visible rejection ratio (R254/R450) of 2 × 105. The seed-induced engineering forecasts its potential application in crystalline Ga2O3 SBPDs under a relatively low processing temperature.
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Affiliation(s)
- Yu Pei
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
| | - Lingyan Liang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
| | - Xiaolong Wang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
| | - Zhenhua Wang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
| | - Hengbo Zhang
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
| | - Junyan Ren
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
| | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, People's Republic of China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
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Abbott R, Abe H, Acernese F, Ackley K, Adhikari N, Adhikari R, Adkins V, Adya V, Affeldt C, Agarwal D, Agathos M, Agatsuma K, Aggarwal N, Aguiar O, Aiello L, Ain A, Ajith P, Akutsu T, Albanesi S, Alfaidi R, Allocca A, Altin P, Amato A, Anand C, Anand S, Ananyeva A, Anderson S, Anderson W, Ando M, Andrade T, Andres N, Andrés-Carcasona M, Andrić T, Angelova S, Ansoldi S, Antelis J, Antier S, Apostolatos T, Appavuravther E, Appert S, Apple S, Arai K, Araya A, Araya M, Areeda J, Arène M, Aritomi N, Arnaud N, Arogeti M, Aronson S, Arun K, Asada H, Asali Y, Ashton G, Aso Y, Assiduo M, Melo SADS, Aston S, Astone P, Aubin F, AultONeal K, Austin C, Babak S, Badaracco F, Bader M, Badger C, Bae S, Bae Y, Baer A, Bagnasco S, Bai Y, Baird J, Bajpai R, Baka T, Ball M, Ballardin G, Ballmer S, Balsamo A, Baltus G, Banagiri S, Banerjee B, Bankar D, Barayoga J, Barbieri C, Barish B, Barker D, Barneo P, Barone F, Barr B, Barsotti L, Barsuglia M, Barta D, Bartlett J, Barton M, Bartos I, Basak S, Bassiri R, Basti A, Bawaj M, Bayley J, Mills J, Milotti E, Minenkov Y, Mio N, Mir L, Miravet-Tenés M, Mishkin A, Mishra C, Mishra T, Mistry T, Bazzan M, Mitra S, Mitrofanov V, Mitselmakher G, Mittleman R, Miyakawa O, Miyo K, Miyoki S, Mo G, Modafferi L, Moguel E, Becher B, Mogushi K, Mohapatra S, Mohite S, Molina I, Molina-Ruiz M, Mondin M, Montani M, Moore C, Moragues J, Moraru D, Bécsy B, Morawski F, More A, Moreno C, Moreno G, Mori Y, Morisaki S, Morisue N, Moriwaki Y, Mours B, Mow-Lowry C, Bedakihale V, Mozzon S, Muciaccia F, Mukherjee A, Mukherjee D, Mukherjee S, Mukherjee S, Mukherjee S, Mukund N, Mullavey A, Munch J, Beirnaert F, Muñiz E, Murray P, Musenich R, Muusse S, Nadji S, Nagano K, Nagar A, Nakamura K, Nakano H, Nakano M, Bejger M, Nakayama Y, Napolano V, Nardecchia I, Narikawa T, Narola H, Naticchioni L, Nayak B, Nayak R, Neil B, Neilson J, Belahcene I, Nelson A, Nelson T, Nery M, Neubauer P, Neunzert A, Ng K, Ng S, Nguyen C, Nguyen P, Nguyen T, Benedetto V, Quynh LN, Ni J, Ni WT, Nichols S, Nishimoto T, Nishizawa A, Nissanke S, Nitoglia E, Nocera F, Norman M, Beniwal D, North C, Nozaki S, Nurbek G, Nuttall L, Obayashi Y, Oberling J, O’Brien B, O’Dell J, Oelker E, Ogaki W, Benjamin M, Oganesyan G, Oh J, Oh K, Oh S, Ohashi M, Ohashi T, Ohkawa M, Ohme F, Ohta H, Okada M, Bennett T, Okutani Y, Olivetto C, Oohara K, Oram R, O’Reilly B, Ormiston R, Ormsby N, O’Shaughnessy R, O’Shea E, Oshino S, Bentley J, Ossokine S, Osthelder C, Otabe S, Ottaway D, Overmier H, Pace A, Pagano G, Pagano R, Page M, Pagliaroli G, BenYaala M, Pai A, Pai S, Pal S, Palamos J, Palashov O, Palomba C, Pan H, Pan KC, Panda P, Pang P, Bera S, Pankow C, Pannarale F, Pant B, Panther F, Paoletti F, Paoli A, Paolone A, Pappas G, Parisi A, Park H, Berbel M, Park J, Parker W, Pascucci D, Pasqualetti A, Passaquieti R, Passuello D, Patel M, Pathak M, Patricelli B, Patron A, Bergamin F, Paul S, Payne E, Pedraza M, Pedurand R, Pegoraro M, Pele A, Arellano FP, Penano S, Penn S, Perego A, Berger B, Pereira A, Pereira T, Perez C, Périgois C, Perkins C, Perreca A, Perriès S, Pesios D, Petermann J, Petterson D, Bernuzzi S, Pfeiffer H, Pham H, Pham K, Phukon K, Phurailatpam H, Piccinni O, Pichot M, Piendibene M, Piergiovanni F, Pierini L, Bersanetti D, Pierro V, Pillant G, Pillas M, Pilo F, Pinard L, Pineda-Bosque C, Pinto I, Pinto M, Piotrzkowski B, Piotrzkowski K, Bertolini A, Pirello M, Pitkin M, Placidi A, Placidi E, Planas M, Plastino W, Pluchar C, Poggiani R, Polini E, Pong D, Betzwieser J, Ponrathnam S, Porter E, Poulton R, Poverman A, Powell J, Pracchia M, Pradier T, Prajapati A, Prasai K, Prasanna R, Beveridge D, Pratten G, Principe M, Prodi G, Prokhorov L, Prosposito P, Prudenzi L, Puecher A, Punturo M, Puosi F, Puppo P, Bhandare R, Pürrer M, Qi H, Quartey N, Quetschke V, Quinonez P, Quitzow-James R, Raab F, Raaijmakers G, Radkins H, Radulesco N, Bhandari A, Raffai P, Rail S, Raja S, Rajan C, Ramirez K, Ramirez T, Ramos-Buades A, Rana J, Rapagnani P, Ray A, Bhardwaj U, Raymond V, Raza N, Razzano M, Read J, Rees L, Regimbau T, Rei L, Reid S, Reid S, Reitze D, Bhatt R, Relton P, Renzini A, Rettegno P, Revenu B, Reza A, Rezac M, Ricci F, Richards D, Richardson J, Richardson L, Bhattacharjee D, Riemenschneider G, Riles K, Rinaldi S, Rink K, Robertson N, Robie R, Robinet F, Rocchi A, Rodriguez S, Rolland L, Bhaumik S, Rollins J, Romanelli M, Romano R, Romel C, Romero A, Romero-Shaw I, Romie J, Ronchini S, Rosa L, Rose C, Bianchi A, Rosińska D, Ross M, Rowan S, Rowlinson S, Roy S, Roy S, Rozza D, Ruggi P, Ruiz-Rocha K, Ryan K, Bilenko I, Sachdev S, Sadecki T, Sadiq J, Saha S, Saito Y, Sakai K, Sakellariadou M, Sakon S, Salafia O, Salces-Carcoba F, Billingsley G, Salconi L, Saleem M, Salemi F, Samajdar A, Sanchez E, Sanchez J, Sanchez L, Sanchis-Gual N, Sanders J, Sanuy A, Bini S, Saravanan T, Sarin N, Sassolas B, Satari H, Sauter O, Savage R, Savant V, Sawada T, Sawant H, Sayah S, Birney R, Schaetzl D, Scheel M, Scheuer J, Schiworski M, Schmidt P, Schmidt S, Schnabel R, Schneewind M, Schofield R, Schönbeck A, Birnholtz O, Schulte B, Schutz B, Schwartz E, Scott J, Scott S, Seglar-Arroyo M, Sekiguchi Y, Sellers D, Sengupta A, Sentenac D, Biscans S, Seo E, Sequino V, Sergeev A, Setyawati Y, Shaffer T, Shahriar M, Shaikh M, Shams B, Shao L, Sharma A, Bischi M, Sharma P, Shawhan P, Shcheblanov N, Sheela A, Shikano Y, Shikauchi M, Shimizu H, Shimode K, Shinkai H, Shishido T, Biscoveanu S, Shoda A, Shoemaker D, Shoemaker D, ShyamSundar S, Sieniawska M, Sigg D, Silenzi L, Singer L, Singh D, Singh M, Bisht A, Singh N, Singha A, Sintes A, Sipala V, Skliris V, Slagmolen B, Slaven-Blair T, Smetana J, Smith J, Smith L, Biswas B, Smith R, Soldateschi J, Somala S, Somiya K, Song I, Soni K, Soni S, Sordini V, Sorrentino F, Sorrentino N, Bitossi M, Soulard R, Souradeep T, Sowell E, Spagnuolo V, Spencer A, Spera M, Spinicelli P, Srivastava A, Srivastava V, Staats K, Bizouard MA, Stachie C, Stachurski F, Steer D, Steinlechner J, Steinlechner S, Stergioulas N, Stops D, Stover M, Strain K, Strang L, Blackburn J, Stratta G, Strong M, Strunk A, Sturani R, Stuver A, Suchenek M, Sudhagar S, Sudhir V, Sugimoto R, Suh H, Blair C, Sullivan A, Summerscales T, Sun L, Sunil S, Sur A, Suresh J, Sutton P, Suzuki T, Suzuki T, Suzuki T, Blair D, Swinkels B, Szczepańczyk M, Szewczyk P, Tacca M, Tagoshi H, Tait S, Takahashi H, Takahashi R, Takano S, Takeda H, Blair R, Takeda M, Talbot C, Talbot C, Tanaka K, Tanaka T, Tanaka T, Tanasijczuk A, Tanioka S, Tanner D, Tao D, Bobba F, Tao L, Tapia R, Martín ETS, Taranto C, Taruya A, Tasson J, Tenorio R, Terhune J, Terkowski L, Thirugnanasambandam M, Bode N, Thomas M, Thomas P, Thompson E, Thompson J, Thondapu S, Thorne K, Thrane E, Tiwari S, Tiwari S, Tiwari V, Boër M, Toivonen A, Tolley A, Tomaru T, Tomura T, Tonelli M, Tornasi Z, Torres-Forné A, Torrie C, e Melo IT, Töyrä D, Bogaert G, Trapananti A, Travasso F, Traylor G, Trevor M, Tringali M, Tripathee A, Troiano L, Trovato A, Trozzo L, Trudeau R, 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Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.042003] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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RL, Warner J, Was M, Washington NY, Watchi J, Weaver B, Webster SA, Weinert M, Weinstein AJ, Weiss R, Weller CM, Wellmann F, Wen L, Weßels P, Wette K, Whelan JT, White DD, Whiting BF, Whittle C, Wilken D, Williams D, Williams MJ, Williamson AR, Willis JL, Willke B, Wilson DJ, Winkler W, Wipf CC, Wlodarczyk T, Woan G, Woehler J, Wofford JK, Wong ICF, Wu DS, Wysocki DM, Xiao L, Yamamoto H, Yang FW, Yang L, Yang Y, Yang Z, Yap MJ, Yeeles DW, Yelikar AB, Ying M, Yoo J, Yu H, Yu H, Zadrożny A, Zanolin M, Zelenova T, Zendri JP, Zevin M, Zhang J, Zhang L, Zhang T, Zhang Y, Zhao C, Zhao G, Zhao Y, Zhou R, Zhou Z, Zhu XJ, Zimmerman AB, Zucker ME, Zweizig J, Jeong D, Shandera S. Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO's and Advanced Virgo's Third Observing Run. Phys Rev Lett 2022; 129:061104. [PMID: 36018635 DOI: 10.1103/physrevlett.129.061104] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/01/2021] [Revised: 03/18/2022] [Accepted: 06/07/2022] [Indexed: 06/15/2023]
Abstract
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 M_{⊙} and 1.0 M_{⊙} in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend our previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio q≥0.1. We do not report any gravitational-wave candidates. The most significant trigger has a false alarm rate of 0.14 yr^{-1}. This implies an upper limit on the merger rate of subsolar binaries in the range [220-24200] Gpc^{-3} yr^{-1}, depending on the chirp mass of the binary. We use this upper limit to derive astrophysical constraints on two phenomenological models that could produce subsolar-mass compact objects. One is an isotropic distribution of equal-mass primordial black holes. Using this model, we find that the fraction of dark matter in primordial black holes in the mass range 0.2 M_{⊙}<m_{PBH}<1.0 M_{⊙} is f_{PBH}≡Ω_{PBH}/Ω_{DM}≲6%. This improves existing constraints on primordial black hole abundance by a factor of ∼3. The other is a dissipative dark matter model, in which fermionic dark matter can collapse and form black holes. The upper limit on the fraction of dark matter black holes depends on the minimum mass of the black holes that can be formed: the most constraining result is obtained at M_{min}=1 M_{⊙}, where f_{DBH}≡Ω_{DBH}/Ω_{DM}≲0.003%. These are the first constraints placed on dissipative dark models by subsolar-mass analyses.
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Affiliation(s)
- R Abbott
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - T D Abbott
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - F Acernese
- Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - K Ackley
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - C Adams
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Adhikari
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - R X Adhikari
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - V B Adya
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - C Affeldt
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Agarwal
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M Agathos
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - K Agatsuma
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - N Aggarwal
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - O D Aguiar
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - L Aiello
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Ain
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - P Ajith
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - S Albanesi
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - A Allocca
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - P A Altin
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Amato
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - C Anand
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - S Anand
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Ananyeva
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S B Anderson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - W G Anderson
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T Andrade
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - N Andres
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - T Andrić
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - S V Angelova
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - S Ansoldi
- Dipartimento di Scienze Matematiche, Informatiche e Fisiche, Università di Udine, I-33100 Udine, Italy
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
| | - J M Antelis
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - S Antier
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - S Appert
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - K Arai
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Araya
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J S Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - M Arène
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - N Arnaud
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S M Aronson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - K G Arun
- Chennai Mathematical Institute, Chennai 603103, India
| | - Y Asali
- Columbia University, New York, New York 10027, USA
| | - G Ashton
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Assiduo
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S M Aston
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - F Aubin
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C Austin
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Babak
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - F Badaracco
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - M K M Bader
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - C Badger
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - S Bae
- Korea Institute of Science and Technology Information, Daejeon 34141, Republic of Korea
| | - A M Baer
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - S Bagnasco
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - Y Bai
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J Baird
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - M Ball
- University of Oregon, Eugene, Oregon 97403, USA
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S W Ballmer
- Syracuse University, Syracuse, New York 13244, USA
| | - A Balsamo
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - G Baltus
- Université de Liège, B-4000 Liège, Belgium
| | - S Banagiri
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - D Bankar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - J C Barayoga
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Barbieri
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - B C Barish
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barker
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Barneo
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - F Barone
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Dipartimento di Medicina, Chirurgia e Odontoiatria "Scuola Medica Salernitana," Università di Salerno, I-84081 Baronissi, Salerno, Italy
| | - B Barr
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Barsotti
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Barsuglia
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - D Barta
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - J Bartlett
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M A Barton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I Bartos
- University of Florida, Gainesville, Florida 32611, USA
| | - R Bassiri
- Stanford University, Stanford, California 94305, USA
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - M Bawaj
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - J C Bayley
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A C Baylor
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Bazzan
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - B Bécsy
- Montana State University, Bozeman, Montana 59717, USA
| | - V M Bedakihale
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - M Bejger
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - I Belahcene
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - V Benedetto
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
| | - D Beniwal
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - T F Bennett
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - J D Bentley
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M BenYaala
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - F Bergamin
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B K Berger
- Stanford University, Stanford, California 94305, USA
| | - S Bernuzzi
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - C P L Berry
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | | | - A Bertolini
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - J Betzwieser
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D Beveridge
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - R Bhandare
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - U Bhardwaj
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - D Bhattacharjee
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - S Bhaumik
- University of Florida, Gainesville, Florida 32611, USA
| | - I A Bilenko
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - G Billingsley
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S Bini
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - R Birney
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - O Birnholtz
- Bar-Ilan University, Ramat Gan, 5290002, Israel
| | - S Biscans
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bischi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S Biscoveanu
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Bisht
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B Biswas
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M-A Bizouard
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - J K Blackburn
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C D Blair
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D G Blair
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - R M Blair
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Bobba
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - N Bode
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Boer
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - G Bogaert
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Boldrini
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - L D Bonavena
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - F Bondu
- Université Rennes, CNRS, Institut FOTON-UMR6082, F-3500 Rennes, France
| | - E Bonilla
- Stanford University, Stanford, California 94305, USA
| | - R Bonnand
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - P Booker
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B A Boom
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - R Bork
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - N Bose
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - S Bose
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Bossilkov
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - V Boudart
- Université de Liège, B-4000 Liège, Belgium
| | - Y Bouffanais
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - A Bozzi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A Bramley
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Branch
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Branchesi
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Breschi
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - T Briant
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - J H Briggs
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Brillet
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Brinkmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - P Brockill
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A F Brooks
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J Brooks
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - D D Brown
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - S Brunett
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - G Bruno
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - R Bruntz
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - J Bryant
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - H J Bulten
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - A Buonanno
- University of Maryland, College Park, Maryland 20742, USA
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - R Buscicchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - D Buskulic
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C Buy
- L2IT, Laboratoire des 2 Infinis-Toulouse, Université de Toulouse, CNRS/IN2P3, UPS, F-31062 Toulouse Cedex 9, France
| | - R L Byer
- Stanford University, Stanford, California 94305, USA
| | - L Cadonati
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - G Cagnoli
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - C Cahillane
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Calderón Bustillo
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - J D Callaghan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T A Callister
- Stony Brook University, Stony Brook, New York 11794, USA
- Center for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USA
| | - E Calloni
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J Cameron
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J B Camp
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Canepa
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Canevarolo
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Cannavacciuolo
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - K C Cannon
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - H Cao
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - E Capote
- Syracuse University, Syracuse, New York 13244, USA
| | - G Carapella
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J B Carlin
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - M F Carney
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - M Carpinelli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - G Carrillo
- University of Oregon, Eugene, Oregon 97403, USA
| | - G Carullo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - T L Carver
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Casanueva Diaz
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Casentini
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - G Castaldi
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Caudill
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Cavaglià
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - F Cavalier
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Ceasar
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - P Cerdá-Durán
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - W Chaibi
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - K Chakravarti
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | | | - E Champion
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - C-H Chan
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - C Chan
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - C L Chan
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - K Chan
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - K Chandra
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - P Chanial
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S Chao
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - P Charlton
- OzGrav, Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
| | - E A Chase
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - E Chassande-Mottin
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - C Chatterjee
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | | | - Deep Chatterjee
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | | | - S Chaty
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - K Chatziioannou
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - H Y Chen
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Chen
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - X Chen
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Chen
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Chen
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - H Cheng
- University of Florida, Gainesville, Florida 32611, USA
| | - C K Cheong
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - H Y Cheung
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - H Y Chia
- University of Florida, Gainesville, Florida 32611, USA
| | - F Chiadini
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - G Chiarini
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - R Chierici
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | | | - M L Chiofalo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - G Cho
- Seoul National University, Seoul 08826, Republic of Korea
| | - H S Cho
- Pusan National University, Busan 46241, Republic of Korea
| | - R K Choudhary
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Choudhary
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - N Christensen
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - Q Chu
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Chua
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - K W Chung
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - G Ciani
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Ciecielag
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - M Cieślar
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - M Cifaldi
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A A Ciobanu
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - R Ciolfi
- INFN, Sezione di Padova, I-35131 Padova, Italy
- INAF, Osservatorio Astronomico di Padova, I-35122 Padova, Italy
| | - F Cipriano
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A Cirone
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - F Clara
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - E N Clark
- University of Arizona, Tucson, Arizona 85721, USA
| | - J A Clark
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - L Clarke
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - P Clearwater
- OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
| | - S Clesse
- Université libre de Bruxelles, Avenue Franklin Roosevelt 50-1050 Bruxelles, Belgium
| | - F Cleva
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - E Coccia
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - E Codazzo
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - D E Cohen
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - L Cohen
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M Colleoni
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - C G Collette
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - A Colombo
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
| | - M Colpi
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
| | - C M Compton
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - L Conti
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - S J Cooper
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - P Corban
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - I Cordero-Carrión
- Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
| | - S Corezzi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - K R Corley
- Columbia University, New York, New York 10027, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - D Corre
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - A Corsi
- Texas Tech University, Lubbock, Texas 79409, USA
| | - S Cortese
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C A Costa
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - R Cotesta
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - M W Coughlin
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - J-P Coulon
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | | | - B Cousins
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - P Couvares
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D M Coward
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M J Cowart
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Coyne
- University of Rhode Island, Kingston, Rhode Island 02881, USA
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T D Creighton
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - A W Criswell
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M Croquette
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - S G Crowder
- Bellevue College, Bellevue, Washington 98007, USA
| | - J R Cudell
- Université de Liège, B-4000 Liège, Belgium
| | - T J Cullen
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Cumming
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Cummings
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Cunningham
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Cuoco
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
- Scuola Normale Superiore, Piazza dei Cavalieri, 7-56126 Pisa, Italy
| | - M Curyło
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - P Dabadie
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - T Dal Canton
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - S Dall'Osso
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - G Dálya
- MTA-ELTE Astrophysics Research Group, Institute of Physics, Eötvös University, Budapest 1117, Hungary
| | - A Dana
- Stanford University, Stanford, California 94305, USA
| | - L M DaneshgaranBajastani
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - B D'Angelo
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Danilishin
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - K Danzmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - A Dasgupta
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - L E H Datrier
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Datta
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - I Dave
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - M Davier
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - G S Davies
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - D Davis
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Davis
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - E J Daw
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - R Dean
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - D DeBra
- Stanford University, Stanford, California 94305, USA
| | - M Deenadayalan
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - J Degallaix
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - M De Laurentis
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - S Deléglise
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - V Del Favero
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - F De Lillo
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - N De Lillo
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - W Del Pozzo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - L M DeMarchi
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - F De Matteis
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - V D'Emilio
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - N Demos
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Dent
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
| | - A Depasse
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - R De Pietri
- Dipartimento di Scienze Matematiche, Fisiche e Informatiche, Università di Parma, I-43124 Parma, Italy
- INFN, Sezione di Milano Bicocca, Gruppo Collegato di Parma, I-43124 Parma, Italy
| | - R De Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C De Rossi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R DeSalvo
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - R De Simone
- Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M C Díaz
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - M Diaz-Ortiz
- University of Florida, Gainesville, Florida 32611, USA
| | - N A Didio
- Syracuse University, Syracuse, New York 13244, USA
| | - T Dietrich
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C Di Fronzo
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - C Di Giorgio
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - F Di Giovanni
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - M Di Giovanni
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - T Di Girolamo
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - B Ding
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - S Di Pace
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - I Di Palma
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - F Di Renzo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A K Divakarla
- University of Florida, Gainesville, Florida 32611, USA
| | - A Dmitriev
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - Z Doctor
- University of Oregon, Eugene, Oregon 97403, USA
| | - L D'Onofrio
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - F Donovan
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K L Dooley
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Doravari
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - I Dorrington
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - M Drago
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - J C Driggers
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Y Drori
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J-G Ducoin
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - P Dupej
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - O Durante
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - D D'Urso
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - P-A Duverne
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - S E Dwyer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Eassa
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P J Easter
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Ebersold
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - T Eckhardt
- Universität Hamburg, D-22761 Hamburg, Germany
| | - G Eddolls
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B Edelman
- University of Oregon, Eugene, Oregon 97403, USA
| | - T B Edo
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - O Edy
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - A Effler
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Eichholz
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | | | - M Eisenmann
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - R A Eisenstein
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ejlli
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E Engelby
- California State University Fullerton, Fullerton, California 92831, USA
| | - L Errico
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R C Essick
- University of Chicago, Chicago, Illinois 60637, USA
| | - H Estellés
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - D Estevez
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - Z Etienne
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - T Etzel
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Evans
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T M Evans
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B E Ewing
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - V Fafone
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - H Fair
- Syracuse University, Syracuse, New York 13244, USA
| | - S Fairhurst
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A M Farah
- University of Chicago, Chicago, Illinois 60637, USA
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- University of Oregon, Eugene, Oregon 97403, USA
| | - W M Farr
- Stony Brook University, Stony Brook, New York 11794, USA
- Center for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USA
| | - N W Farrow
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - E J Fauchon-Jones
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - G Favaro
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - M Favata
- Montclair State University, Montclair, New Jersey 07043, USA
| | - M Fays
- Université de Liège, B-4000 Liège, Belgium
| | - M Fazio
- Colorado State University, Fort Collins, Colorado 80523, USA
| | - J Feicht
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M M Fejer
- Stanford University, Stanford, California 94305, USA
| | - B Fekecs
- University of Szeged, Dóm tér 9, Szeged 6720, Hungary
| | - E Fenyvesi
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
- Institute for Nuclear Research, Hungarian Academy of Sciences, Bem t'er 18/c, H-4026 Debrecen, Hungary
| | - D L Ferguson
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - A Fernandez-Galiana
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - T A Ferreira
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - P Figura
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Fishbach
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - R P Fisher
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - R Fittipaldi
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- CNR-SPIN, c/o Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - V Fiumara
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Scuola di Ingegneria, Università della Basilicata, I-85100 Potenza, Italy
| | - R Flaminio
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
- Gravitational Wave Science Project, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan
| | - E Floden
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - H Fong
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - J A Font
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
- Observatori Astronòmic, Universitat de València, E-46980 Paterna, València, Spain
| | - B Fornal
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - P W F Forsyth
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Franke
- Universität Hamburg, D-22761 Hamburg, Germany
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | | | - J P Freed
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - Z Frei
- MTA-ELTE Astrophysics Research Group, Institute of Physics, Eötvös University, Budapest 1117, Hungary
| | - A Freise
- Vrije Universiteit Amsterdam, 1081 HV, Amsterdam, Netherlands
| | - R Frey
- University of Oregon, Eugene, Oregon 97403, USA
| | - P Fritschel
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V V Frolov
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G G Fronzé
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H A Gabbard
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B U Gadre
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - J R Gair
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - J Gais
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - S Galaudage
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - R Gamba
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - D Ganapathy
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ganguly
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - S G Gaonkar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - B Garaventa
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - C García-Núñez
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - C García-Quirós
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - F Garufi
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - B Gateley
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Gaudio
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - V Gayathri
- University of Florida, Gainesville, Florida 32611, USA
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - J George
- RRCAT, Indore, Madhya Pradesh 452013, India
| | | | - L Gergely
- University of Szeged, Dóm tér 9, Szeged 6720, Hungary
| | - P Gewecke
- Universität Hamburg, D-22761 Hamburg, Germany
| | - S Ghonge
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - Abhirup Ghosh
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | | | - Shaon Ghosh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
- Montclair State University, Montclair, New Jersey 07043, USA
| | - Shrobana Ghosh
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Giacomazzo
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - L Giacoppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K D Giardina
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D R Gibson
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - C Gier
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - M Giesler
- Cornell University, Ithaca, New York 14850, USA
| | - P Giri
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Gissi
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
| | - J Glanzer
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A E Gleckl
- California State University Fullerton, Fullerton, California 92831, USA
| | - P Godwin
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - E Goetz
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - R Goetz
- University of Florida, Gainesville, Florida 32611, USA
| | - N Gohlke
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B Goncharov
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - G González
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Gopakumar
- Tata Institute of Fundamental Research, Mumbai 400005, India
| | - M Gosselin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Gouaty
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D W Gould
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - B Grace
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Grado
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- INAF, Osservatorio Astronomico di Capodimonte, I-80131 Napoli, Italy
| | - M Granata
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - V Granata
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - A Grant
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Gras
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - P Grassia
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Gray
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Gray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Greco
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - A C Green
- University of Florida, Gainesville, Florida 32611, USA
| | - R Green
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - E M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - D Griffith
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - W Griffiths
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - H L Griggs
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - G Grignani
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - A Grimaldi
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - S J Grimm
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - H Grote
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Grunewald
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - P Gruning
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - D Guerra
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - G M Guidi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - A R Guimaraes
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - G Guixé
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - H K Gulati
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - H-K Guo
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - Y Guo
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - Anchal Gupta
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - Anuradha Gupta
- The University of Mississippi, University, Mississippi 38677, USA
| | - P Gupta
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - E K Gustafson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Gustafson
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - F Guzman
- Texas A&M University, College Station, Texas 77843, USA
| | - L Haegel
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - O Halim
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - E D Hall
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Z Hamilton
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - G Hammond
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Haney
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - J Hanks
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Hanna
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - M D Hannam
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - O Hannuksela
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - H Hansen
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T J Hansen
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J Hanson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Harder
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - T Hardwick
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - K Haris
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - J Harms
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - G M Harry
- American University, Washington, D.C. 20016, USA
| | - I W Harry
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - D Hartwig
- Universität Hamburg, D-22761 Hamburg, Germany
| | - B Haskell
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - R K Hasskew
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - C-J Haster
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F J Hayes
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Healy
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - A Heidmann
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - A Heidt
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M C Heintze
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Heinze
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - J Heinzel
- Carleton College, Northfield, Minnesota 55057, USA
| | - H Heitmann
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - F Hellman
- University of California, Berkeley, California 94720, USA
| | - P Hello
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | | | - G Hemming
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Hendry
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I S Heng
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Hennes
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - J Hennig
- Maastricht University, 6200 MD, Maastricht, Netherlands
| | - M H Hennig
- Maastricht University, 6200 MD, Maastricht, Netherlands
| | - A G Hernandez
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - F Hernandez Vivanco
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Heurs
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Hild
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - P Hill
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - A S Hines
- Texas A&M University, College Station, Texas 77843, USA
| | - S Hochheim
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Hofman
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - J N Hohmann
- Universität Hamburg, D-22761 Hamburg, Germany
| | - D G Holcomb
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - N A Holland
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - I J Hollows
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - Z J Holmes
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - K Holt
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D E Holz
- University of Chicago, Chicago, Illinois 60637, USA
| | - P Hopkins
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Hourihane
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - E J Howell
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - C G Hoy
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - D Hoyland
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - A Hreibi
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - Y Hsu
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - Y Huang
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M T Hübner
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - A D Huddart
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - B Hughey
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - V Hui
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - S Husa
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - S H Huttner
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Huxford
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - T Huynh-Dinh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B Idzkowski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Iess
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - C Ingram
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - M Isi
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K Isleif
- Universität Hamburg, D-22761 Hamburg, Germany
| | - B R Iyer
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - V JaberianHamedan
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - T Jacqmin
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - S J Jadhav
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - S P Jadhav
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - A L James
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Z Jan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - K Jani
- Vanderbilt University, Nashville, Tennessee 37235, USA
| | - J Janquart
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - K Janssens
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
- Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium
| | - N N Janthalur
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - P Jaranowski
- University of Białystok, 15-424 Białystok, Poland
| | - D Jariwala
- University of Florida, Gainesville, Florida 32611, USA
| | - R Jaume
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - A C Jenkins
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - K Jenner
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - M Jeunon
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - W Jia
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G R Johns
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - A W Jones
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D I Jones
- University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - J D Jones
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Jones
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Jones
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R J G Jonker
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - L Ju
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Junker
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - V Juste
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - C V Kalaghatgi
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - V Kalogera
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - B Kamai
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S Kandhasamy
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - G Kang
- Chung-Ang University, Seoul 06974, Republic of Korea
| | - J B Kanner
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - Y Kao
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - S J Kapadia
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - D P Kapasi
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S Karat
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Karathanasis
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - S Karki
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - R Kashyap
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - M Kasprzack
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - W Kastaun
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Katsanevas
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E Katsavounidis
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Katzman
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Kaur
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Kawabe
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Kéfélian
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - D Keitel
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - J S Key
- University of Washington Bothell, Bothell, Washington 98011, USA
| | - S Khadka
- Stanford University, Stanford, California 94305, USA
| | - F Y Khalili
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - S Khan
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
| | - N Khetan
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | | | - N Kijbunchoo
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - C Kim
- Ewha Womans University, Seoul 03760, Republic of Korea
| | - J C Kim
- Inje University Gimhae, South Gyeongsang 50834, Republic of Korea
| | - K Kim
- Korea Astronomy and Space Science Institute, Daejeon 34055, Republic of Korea
| | - W S Kim
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - Y-M Kim
- Ulsan National Institute of Science and Technology, Ulsan 44919, Republic of Korea
| | - C Kimball
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - M Kinley-Hanlon
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Kirchhoff
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - J S Kissel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L Kleybolte
- Universität Hamburg, D-22761 Hamburg, Germany
| | - S Klimenko
- University of Florida, Gainesville, Florida 32611, USA
| | - A M Knee
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - T D Knowles
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - E Knyazev
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - P Koch
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Koekoek
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S Koley
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - P Kolitsidou
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - M Kolstein
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - K Komori
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V Kondrashov
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Kontos
- Bard College, 30 Campus Road, Annandale-On-Hudson, New York 12504, USA
| | - N Koper
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Korobko
- Universität Hamburg, D-22761 Hamburg, Germany
| | - M Kovalam
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D B Kozak
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kringel
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - N V Krishnendu
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Królak
- Institute of Mathematics, Polish Academy of Sciences, 00656 Warsaw, Poland
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - G Kuehn
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - F Kuei
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - P Kuijer
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - A Kumar
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - P Kumar
- Cornell University, Ithaca, New York 14850, USA
| | - Rahul Kumar
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Rakesh Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - K Kuns
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S Kuwahara
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - P Lagabbe
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D Laghi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - E Lalande
- Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
| | - T L Lam
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - A Lamberts
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
- Laboratoire Lagrange, Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Landry
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B B Lane
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - R N Lang
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Lange
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - I La Rosa
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | | | - P D Lasky
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Laxen
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Lazzarini
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Lazzaro
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - S Leavey
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - Y K Lecoeuche
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - H M Lee
- Seoul National University, Seoul 08826, Republic of Korea
| | - H W Lee
- Inje University Gimhae, South Gyeongsang 50834, Republic of Korea
| | - J Lee
- Seoul National University, Seoul 08826, Republic of Korea
| | - K Lee
- Sungkyunkwan University, Seoul 03063, Republic of Korea
| | - J Lehmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Lemaître
- NAVIER, École des Ponts, Université Gustave Eiffel, CNRS, Marne-la-Vallée, France
| | - N Leroy
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - N Letendre
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C Levesque
- Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
| | - Y Levin
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - J N Leviton
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - K Leyde
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - A K Y Li
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - B Li
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - J Li
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - T G F Li
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - X Li
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - F Linde
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - S D Linker
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - J N Linley
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T B Littenberg
- NASA Marshall Space Flight Center, Huntsville, Alabama 35811, USA
| | - J Liu
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - K Liu
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - X Liu
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Llamas
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - M Llorens-Monteagudo
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - R K L Lo
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Lockwood
- University of Washington, Seattle, Washington 98195, USA
| | - L T London
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Longo
- Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, I-00146 Roma, Italy
- INFN, Sezione di Roma Tre, I-00146 Roma, Italy
| | - D Lopez
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - M Lopez Portilla
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Lorenzini
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - M Lormand
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G Losurdo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - T P Lott
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - J D Lough
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C O Lousto
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - G Lovelace
- California State University Fullerton, Fullerton, California 92831, USA
| | | | - H Lück
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Lumaca
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A P Lundgren
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J E Lynam
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - R Macas
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - M MacInnis
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Macleod
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - I A O MacMillan
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Macquet
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | | | - C Magazzù
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - R M Magee
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Maggiore
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Magnozzi
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Mahesh
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - C Makarem
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | | | - S Maliakal
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Malik
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - N Man
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - V Mandic
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - J L Mango
- Concordia University Wisconsin, Mequon, Wisconsin 53097, USA
| | - G L Mansell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Manske
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Mantovani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Mapelli
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
- School of Physics Science and Engineering, Tongji University, Shanghai 200092, China
| | - F Marion
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - Z Mark
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - S Márka
- Columbia University, New York, New York 10027, USA
| | - Z Márka
- Columbia University, New York, New York 10027, USA
| | - C Markakis
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - A S Markosyan
- Stanford University, Stanford, California 94305, USA
| | - A Markowitz
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - E Maros
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Marquina
- Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
| | - S Marsat
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - F Martelli
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - I W Martin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R M Martin
- Montclair State University, Montclair, New Jersey 07043, USA
| | - M Martinez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - V A Martinez
- University of Florida, Gainesville, Florida 32611, USA
| | - V Martinez
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - K Martinovic
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - D V Martynov
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - E J Marx
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | | | - K Mason
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Massera
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - A Masserot
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - T J Massinger
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Masso-Reid
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Mastrogiovanni
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - A Matas
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - M Mateu-Lucena
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - F Matichard
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Matiushechkina
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - N Mavalvala
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J J McCann
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - R McCarthy
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - P K McClincy
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - S McCormick
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L McCuller
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G I McGhee
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - C McIsaac
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J McIver
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - T McRae
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S T McWilliams
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - D Meacher
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Mehmet
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A K Mehta
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - Q Meijer
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - A Melatos
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - D A Melchor
- California State University Fullerton, Fullerton, California 92831, USA
| | - G Mendell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - A Menendez-Vazquez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - C S Menoni
- Colorado State University, Fort Collins, Colorado 80523, USA
| | - R A Mercer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - L Mereni
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - K Merfeld
- University of Oregon, Eugene, Oregon 97403, USA
| | - E L Merilh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J D Merritt
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Merzougui
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - S Meshkov
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Messenger
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Messick
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - P M Meyers
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - F Meylahn
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Mhaske
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - A Miani
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - H Miao
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | | | - C Michel
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - H Middleton
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - L Milano
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Miller
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - A L Miller
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - B Miller
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - M Millhouse
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - J C Mills
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E Milotti
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - O Minazzoli
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
- Centre Scientifique de Monaco, 8 quai Antoine Ier, MC-98000, Monaco
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - Ll M Mir
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - M Miravet-Tenés
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - C Mishra
- Indian Institute of Technology Madras, Chennai 600036, India
| | - T Mishra
- University of Florida, Gainesville, Florida 32611, USA
| | - T Mistry
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - S Mitra
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V P Mitrofanov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | | | - R Mittleman
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Geoffrey Mo
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Moguel
- Kenyon College, Gambier, Ohio 43022, USA
| | - K Mogushi
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - S R P Mohapatra
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S R Mohite
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - I Molina
- California State University Fullerton, Fullerton, California 92831, USA
| | - M Molina-Ruiz
- University of California, Berkeley, California 94720, USA
| | - M Mondin
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - M Montani
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - C J Moore
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - D Moraru
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Morawski
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - A More
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - C Moreno
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - G Moreno
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Morisaki
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - B Mours
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - C M Mow-Lowry
- University of Birmingham, Birmingham B15 2TT, United Kingdom
- Vrije Universiteit Amsterdam, 1081 HV, Amsterdam, Netherlands
| | - S Mozzon
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - F Muciaccia
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - Arunava Mukherjee
- Saha Institute of Nuclear Physics, Bidhannagar, West Bengal 700064, India
| | - D Mukherjee
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - Soma Mukherjee
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | | | - Suvodip Mukherjee
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - N Mukund
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Mullavey
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Munch
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - E A Muñiz
- Syracuse University, Syracuse, New York 13244, USA
| | - P G Murray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Musenich
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Muusse
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - S L Nadji
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Nagar
- INFN Sezione di Torino, I-10125 Torino, Italy
- Institut des Hautes Etudes Scientifiques, F-91440 Bures-sur-Yvette, France
| | - V Napolano
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - I Nardecchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - B Nayak
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - R K Nayak
- Indian Institute of Science Education and Research, Kolkata, Mohanpur, West Bengal 741252, India
| | - B F Neil
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Neilson
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Nelemans
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, Netherlands
| | - T J N Nelson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Nery
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - P Neubauer
- Kenyon College, Gambier, Ohio 43022, USA
| | - A Neunzert
- University of Washington Bothell, Bothell, Washington 98011, USA
| | - K Y Ng
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S W S Ng
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - C Nguyen
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - P Nguyen
- University of Oregon, Eugene, Oregon 97403, USA
| | - T Nguyen
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S A Nichols
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Nissanke
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - E Nitoglia
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Norman
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - C North
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - L K Nuttall
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J Oberling
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B D O'Brien
- University of Florida, Gainesville, Florida 32611, USA
| | - J O'Dell
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - E Oelker
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Oganesyan
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - J J Oh
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - S H Oh
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - F Ohme
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - H Ohta
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - M A Okada
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - C Olivetto
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Oram
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B O'Reilly
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - R G Ormiston
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - N D Ormsby
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - L F Ortega
- University of Florida, Gainesville, Florida 32611, USA
| | - R O'Shaughnessy
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - E O'Shea
- Cornell University, Ithaca, New York 14850, USA
| | - S Ossokine
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - C Osthelder
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D J Ottaway
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - H Overmier
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A E Pace
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - G Pagano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - M A Page
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Pagliaroli
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - A Pai
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - S A Pai
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - J R Palamos
- University of Oregon, Eugene, Oregon 97403, USA
| | - O Palashov
- Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
| | - C Palomba
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - H Pan
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - P K Panda
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - P T H Pang
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - C Pankow
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - F Pannarale
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - B C Pant
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - F H Panther
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - A Paoli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Paolone
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Consiglio Nazionale delle Ricerche-Istituto dei Sistemi Complessi, Piazzale Aldo Moro 5, I-00185 Roma, Italy
| | - H Park
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - W Parker
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - D Pascucci
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | | | - M Patel
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - M Pathak
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - B Patricelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A S Patron
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Paul
- University of Oregon, Eugene, Oregon 97403, USA
| | - E Payne
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Pedraza
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Pegoraro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - A Pele
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Penn
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - A Perego
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - A Pereira
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - T Pereira
- International Institute of Physics, Universidade Federal do Rio Grande do Norte, Natal RN 59078-970, Brazil
| | - C J Perez
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Périgois
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C C Perkins
- University of Florida, Gainesville, Florida 32611, USA
| | - A Perreca
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - S Perriès
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - J Petermann
- Universität Hamburg, D-22761 Hamburg, Germany
| | - D Petterson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - H P Pfeiffer
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - K A Pham
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - K S Phukon
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | | | - M Pichot
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Piendibene
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Piergiovanni
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - L Pierini
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - V Pierro
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Pillant
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Pillas
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - F Pilo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - L Pinard
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - I M Pinto
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi," I-00184 Roma, Italy
| | - M Pinto
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Piotrzkowski
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - M Pirello
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M D Pitkin
- Lancaster University, Lancaster LA1 4YW, United Kingdom
| | - E Placidi
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - L Planas
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - W Plastino
- Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, I-00146 Roma, Italy
- INFN, Sezione di Roma Tre, I-00146 Roma, Italy
| | - C Pluchar
- University of Arizona, Tucson, Arizona 85721, USA
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - E Polini
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D Y T Pong
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - S Ponrathnam
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - P Popolizio
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E K Porter
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - R Poulton
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Powell
- OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
| | - M Pracchia
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - T Pradier
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - A K Prajapati
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - K Prasai
- Stanford University, Stanford, California 94305, USA
| | - R Prasanna
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - G Pratten
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Principe
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi," I-00184 Roma, Italy
| | - G A Prodi
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
- Università di Trento, Dipartimento di Matematica, I-38123 Povo, Trento, Italy
| | - L Prokhorov
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - P Prosposito
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Prudenzi
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - A Puecher
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - F Puosi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - M Pürrer
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - H Qi
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - V Quetschke
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - R Quitzow-James
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - F J Raab
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - G Raaijmakers
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - H Radkins
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - N Radulesco
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - P Raffai
- MTA-ELTE Astrophysics Research Group, Institute of Physics, Eötvös University, Budapest 1117, Hungary
| | - S X Rail
- Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
| | - S Raja
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - C Rajan
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - K E Ramirez
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T D Ramirez
- California State University Fullerton, Fullerton, California 92831, USA
| | - A Ramos-Buades
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - J Rana
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - U D Rapol
- Indian Institute of Science Education and Research, Pune, Maharashtra 411008, India
| | - A Ray
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - V Raymond
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - N Raza
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - J Read
- California State University Fullerton, Fullerton, California 92831, USA
| | - L A Rees
- American University, Washington, D.C. 20016, USA
| | - T Regimbau
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - L Rei
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - S Reid
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - S W Reid
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - D H Reitze
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- University of Florida, Gainesville, Florida 32611, USA
| | - P Relton
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Renzini
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - P Rettegno
- INFN Sezione di Torino, I-10125 Torino, Italy
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy
| | - M Rezac
- California State University Fullerton, Fullerton, California 92831, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - D Richards
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - J W Richardson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - L Richardson
- Texas A&M University, College Station, Texas 77843, USA
| | - G Riemenschneider
- INFN Sezione di Torino, I-10125 Torino, Italy
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy
| | - K Riles
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - S Rinaldi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - K Rink
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - M Rizzo
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - N A Robertson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Robie
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - F Robinet
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Rodriguez
- California State University Fullerton, Fullerton, California 92831, USA
| | - L Rolland
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - J G Rollins
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Romanelli
- Université Rennes, CNRS, Institut FOTON-UMR6082, F-3500 Rennes, France
| | - R Romano
- Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C L Romel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - A Romero-Rodríguez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - I M Romero-Shaw
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - J H Romie
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Ronchini
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - L Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C A Rose
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Rosińska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - M P Ross
- University of Washington, Seattle, Washington 98195, USA
| | - S Rowan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S J Rowlinson
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Roy
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - Santosh Roy
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - Soumen Roy
- Indian Institute of Technology, Palaj, Gandhinagar, Gujarat 382355, India
| | - D Rozza
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Ryan
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Sachdev
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - T Sadecki
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Sadiq
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
| | - M Sakellariadou
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - O S Salafia
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - L Salconi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Saleem
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F Salemi
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - A Samajdar
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - E J Sanchez
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J H Sanchez
- California State University Fullerton, Fullerton, California 92831, USA
| | - L E Sanchez
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - N Sanchis-Gual
- Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications, Campus de Santiago, 3810-183 Aveiro, Portugal
| | - J R Sanders
- Marquette University, 11420 W. Clybourn Street, Milwaukee, Wisconsin 53233, USA
| | - A Sanuy
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - T R Saravanan
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - N Sarin
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - B Sassolas
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - H Satari
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - B S Sathyaprakash
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - O Sauter
- University of Florida, Gainesville, Florida 32611, USA
| | - R L Savage
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D Sawant
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - H L Sawant
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - S Sayah
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - D Schaetzl
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Scheel
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - J Scheuer
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - M Schiworski
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - P Schmidt
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Schmidt
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - R Schnabel
- Universität Hamburg, D-22761 Hamburg, Germany
| | - M Schneewind
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - A Schönbeck
- Universität Hamburg, D-22761 Hamburg, Germany
| | - B W Schulte
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B F Schutz
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E Schwartz
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - M Seglar-Arroyo
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D Sellers
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A S Sengupta
- Indian Institute of Technology, Palaj, Gandhinagar, Gujarat 382355, India
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E G Seo
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - V Sequino
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
| | - Y Setyawati
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - T Shaffer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M S Shahriar
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - B Shams
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - A Sharma
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - P Sharma
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - P Shawhan
- University of Maryland, College Park, Maryland 20742, USA
| | - N S Shcheblanov
- NAVIER, École des Ponts, Université Gustave Eiffel, CNRS, Marne-la-Vallée, France
| | - M Shikauchi
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - D H Shoemaker
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Shoemaker
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | | | - M Sieniawska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - D Sigg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L P Singer
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - D Singh
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - N Singh
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Singha
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - A M Sintes
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - V Sipala
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - V Skliris
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B J J Slagmolen
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - T J Slaven-Blair
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Smetana
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - R J E Smith
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - J Soldateschi
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
- Università di Firenze, Sesto Fiorentino I-50019, Italy
- INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
| | - S N Somala
- Indian Institute of Technology Hyderabad, Sangareddy, Khandi, Telangana 502285, India
| | - E J Son
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - K Soni
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - S Soni
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - V Sordini
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | | | - N Sorrentino
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - R Soulard
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - T Souradeep
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
- Indian Institute of Science Education and Research, Pune, Maharashtra 411008, India
| | - E Sowell
- Texas Tech University, Lubbock, Texas 79409, USA
| | - V Spagnuolo
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - A P Spencer
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Spera
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - R Srinivasan
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A K Srivastava
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - V Srivastava
- Syracuse University, Syracuse, New York 13244, USA
| | - K Staats
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - C Stachie
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - D A Steer
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - J Steinlechner
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S Steinlechner
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S Stevenson
- OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
| | - D J Stops
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Stover
- Kenyon College, Gambier, Ohio 43022, USA
| | - K A Strain
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L C Strang
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - G Stratta
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
- INAF, Osservatorio di Astrofisica e Scienza dello Spazio, I-40129 Bologna, Italy
| | - A Strunk
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Sturani
- International Institute of Physics, Universidade Federal do Rio Grande do Norte, Natal RN 59078-970, Brazil
| | - A L Stuver
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - S Sudhagar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Sudhir
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - H G Suh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | | | - H Sun
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - L Sun
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S Sunil
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - A Sur
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - J Suresh
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - P J Sutton
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B L Swinkels
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | | | - P Szewczyk
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - M Tacca
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - S C Tait
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C J Talbot
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - C Talbot
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A J Tanasijczuk
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - D Tao
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - L Tao
- University of Florida, Gainesville, Florida 32611, USA
| | | | - C Taranto
- Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - J D Tasson
- Carleton College, Northfield, Minnesota 55057, USA
| | - R Tenorio
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - J E Terhune
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - L Terkowski
- Universität Hamburg, D-22761 Hamburg, Germany
| | | | - M Thomas
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Thomas
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J E Thompson
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | | | - K A Thorne
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - E Thrane
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - Shubhanshu Tiwari
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - Srishti Tiwari
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Tiwari
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A M Toivonen
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - K Toland
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A E Tolley
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A Torres-Forné
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - C I Torrie
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - I Tosta E Melo
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - D Töyrä
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Trapananti
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - G Traylor
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Trevor
- University of Maryland, College Park, Maryland 20742, USA
| | - M C Tringali
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Tripathee
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - L Troiano
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Dipartimento di Scienze Aziendali-Management and Innovation Systems (DISA-MIS), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - A Trovato
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - L Trozzo
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R J Trudeau
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D S Tsai
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - D Tsai
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - K W Tsang
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
- Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, Netherlands
| | - M Tse
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - R Tso
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - L Tsukada
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - D Tsuna
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - T Tsutsui
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - K Turbang
- Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium
- Vrije Universiteit Brussel, Boulevard de la Plaine 2, 1050 Ixelles, Belgium
| | - M Turconi
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A S Ubhi
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R P Udall
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - K Ueno
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | | | - A L Urban
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Utina
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - H Vahlbruch
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Vajente
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Vajpeyi
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - G Valdes
- Texas A&M University, College Station, Texas 77843, USA
| | - M Valentini
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - V Valsan
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - N van Bakel
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - M van Beuzekom
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - J F J van den Brand
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
- Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - C Van Den Broeck
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | | | | | | | - J Vanosky
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - N van Remortel
- Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium
| | - M Vardaro
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - A F Vargas
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - V Varma
- Cornell University, Ithaca, New York 14850, USA
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - A Vecchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - J Veitch
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P J Veitch
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - J Venneberg
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Venugopalan
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D Verkindt
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - P Verma
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - Y Verma
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - D Veske
- Columbia University, New York, New York 10027, USA
| | - F Vetrano
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - A Viceré
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S Vidyant
- Syracuse University, Syracuse, New York 13244, USA
| | - A D Viets
- Concordia University Wisconsin, Mequon, Wisconsin 53097, USA
| | - A Vijaykumar
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - V Villa-Ortega
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
| | - J-Y Vinet
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A Virtuoso
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - S Vitale
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Vo
- Syracuse University, Syracuse, New York 13244, USA
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - E R G von Reis
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J S A von Wrangel
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C Vorvick
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S P Vyatchanin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - L E Wade
- Kenyon College, Gambier, Ohio 43022, USA
| | - M Wade
- Kenyon College, Gambier, Ohio 43022, USA
| | - K J Wagner
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - R C Walet
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - M Walker
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - G S Wallace
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - L Wallace
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S Walsh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - J Z Wang
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - W H Wang
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - R L Ward
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - J Warner
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Was
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - N Y Washington
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J Watchi
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - B Weaver
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S A Webster
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Weinert
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A J Weinstein
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Weiss
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - C M Weller
- University of Washington, Seattle, Washington 98195, USA
| | - F Wellmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - L Wen
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Weßels
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - K Wette
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - J T Whelan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - D D White
- California State University Fullerton, Fullerton, California 92831, USA
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - C Whittle
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D Wilken
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Williams
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M J Williams
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A R Williamson
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J L Willis
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - B Willke
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D J Wilson
- University of Arizona, Tucson, Arizona 85721, USA
| | - W Winkler
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C C Wipf
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - T Wlodarczyk
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - G Woan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Woehler
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - J K Wofford
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - I C F Wong
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - D S Wu
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D M Wysocki
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - L Xiao
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - H Yamamoto
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - F W Yang
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - L Yang
- Colorado State University, Fort Collins, Colorado 80523, USA
| | - Yang Yang
- University of Florida, Gainesville, Florida 32611, USA
| | - Z Yang
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M J Yap
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - D W Yeeles
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A B Yelikar
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - M Ying
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - J Yoo
- Cornell University, Ithaca, New York 14850, USA
| | - Hang Yu
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - Haocun Yu
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Zadrożny
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - M Zanolin
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - T Zelenova
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - M Zevin
- University of Chicago, Chicago, Illinois 60637, USA
| | - J Zhang
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - L Zhang
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - T Zhang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - Y Zhang
- Texas A&M University, College Station, Texas 77843, USA
| | - C Zhao
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Zhao
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - Yue Zhao
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - R Zhou
- University of California, Berkeley, California 94720, USA
| | - Z Zhou
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - X J Zhu
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - A B Zimmerman
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - M E Zucker
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Zweizig
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - Donghui Jeong
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - Sarah Shandera
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
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Abbott R, Abbott T, Acernese F, Ackley K, Adams C, Adhikari N, Adhikari R, Adya V, Affeldt C, Agarwal D, Agathos M, Agatsuma K, Aggarwal N, Aguiar O, Aiello L, Ain A, Ajith P, Akutsu T, Albanesi S, Allocca A, Altin P, Amato A, Anand C, Anand S, Ananyeva A, Anderson S, Anderson W, Ando M, Andrade T, Andres N, Andrić T, Angelova S, Ansoldi S, Antelis J, Antier S, Appert S, Arai K, Arai K, Arai Y, Araki S, Araya A, Araya M, Areeda J, Arène M, Aritomi N, Arnaud N, Aronson S, Arun K, Asada H, Asali Y, Ashton G, Aso Y, Assiduo M, Aston S, Astone P, Aubin F, Austin C, Babak S, Badaracco F, Bader M, Badger C, Bae S, Bae Y, Baer A, Bagnasco S, Bai Y, Baiotti L, Baird J, Bajpai R, Ball M, Ballardin G, Ballmer S, Balsamo A, Baltus G, Banagiri S, Bankar D, Barayoga J, Barbieri C, Barish B, Barker D, Barneo P, Barone F, Barr B, Barsotti L, Barsuglia M, Barta D, Bartlett J, Barton M, Bartos I, Bassiri R, Basti A, Bawaj M, Bayley J, Baylor A, Bazzan M, Bécsy B, Bedakihale V, Bejger M, Belahcene I, Benedetto V, Moreno G, Mori Y, Morisaki S, Moriwaki Y, Mours B, Mow-Lowry C, Mozzon S, Muciaccia F, Mukherjee A, Mukherjee D, Beniwal D, Mukherjee S, Mukherjee S, Mukherjee S, Mukund N, Mullavey A, Munch J, Muñiz E, Murray P, Musenich R, Muusse S, Bennett T, Nadji S, Nagano K, Nagano S, Nagar A, Nakamura K, Nakano H, Nakano M, Nakashima R, Nakayama Y, Napolano V, Bentley J, Nardecchia I, Narikawa T, Naticchioni L, Nayak B, Nayak R, Negishi R, Neil B, Neilson J, Nelemans G, Nelson T, BenYaala M, Nery M, Neubauer P, Neunzert A, Ng K, Ng S, Nguyen C, Nguyen P, Nguyen T, Quynh LN, Ni WT, Bergamin F, Nichols S, Nishizawa A, Nissanke S, Nitoglia E, Nocera F, Norman M, North C, Nozaki S, Nuttall L, Oberling J, Berger B, O’Brien B, Obuchi Y, O’Dell J, Oelker E, Ogaki W, Oganesyan G, Oh J, Oh K, Oh S, Ohashi M, Bernuzzi S, Ohishi N, Ohkawa M, Ohme F, Ohta H, Okada M, Okutani Y, Okutomi K, Olivetto C, Oohara K, Ooi C, Bersanetti D, Oram R, O’Reilly B, Ormiston R, Ormsby N, Ortega L, O’Shaughnessy R, O’Shea E, Oshino S, Ossokine S, Osthelder C, Bertolini A, Otabe S, Ottaway D, Overmier H, Pace A, Pagano G, Page M, Pagliaroli G, Pai A, Pai S, Palamos J, Betzwieser J, Palashov O, Palomba C, Pan H, Pan K, Panda P, Pang H, Pang P, Pankow C, Pannarale F, Pant B, Beveridge D, Panther F, Paoletti F, Paoli A, Paolone A, Parisi A, Park H, Park J, Parker W, Pascucci D, Pasqualetti A, Bhandare R, Passaquieti R, Passuello D, Patel M, Pathak M, Patricelli B, Patron A, Paul S, Payne E, Pedraza M, Pegoraro M, Bhardwaj U, Pele A, Arellano FP, Penn S, Perego A, Pereira A, Pereira T, Perez C, Périgois C, Perkins C, Perreca A, Bhattacharjee D, Perriès S, Petermann J, Petterson D, Pfeiffer H, Pham K, Phukon K, Piccinni O, Pichot M, Piendibene M, Piergiovanni F, Bhaumik S, Pierini L, Pierro V, Pillant G, Pillas M, Pilo F, Pinard L, Pinto I, Pinto M, Piotrzkowski K, Pirello M, Bilenko I, Pitkin M, Placidi E, Planas L, Plastino W, Pluchar C, Poggiani R, Polini E, Pong D, Ponrathnam S, Popolizio P, Billingsley G, Porter E, Poulton R, Powell J, Pracchia M, Pradier T, Prajapati A, Prasai K, Prasanna R, Pratten G, Principe M, Bini S, Prodi G, Prokhorov L, Prosposito P, Prudenzi L, Puecher A, Punturo M, Puosi F, Puppo P, Pürrer M, Qi H, Birney R, Quetschke V, Quitzow-James R, Raab F, Raaijmakers G, Radkins H, Radulesco N, Raffai P, Rail S, Raja S, Rajan C, Birnholtz O, Ramirez K, Ramirez T, Ramos-Buades A, Rana J, Rapagnani P, Rapol U, Ray A, Raymond V, Raza N, Razzano M, Biscans S, Read J, Rees L, Regimbau T, Rei L, Reid S, Reid S, Reitze D, Relton P, Renzini A, Rettegno P, Bischi M, Rezac M, Ricci F, Richards D, Richardson J, Richardson L, Riemenschneider G, Riles K, Rinaldi S, Rink K, Rizzo M, Biscoveanu S, Robertson N, Robie R, Robinet F, Rocchi A, Rodriguez S, Rolland L, Rollins J, Romanelli M, Romano J, Romano R, Bisht A, Romel C, Romero-Rodríguez A, Romero-Shaw I, Romie J, Ronchini S, Rosa L, Rose C, Rosińska D, Ross M, Rowan S, Biswas B, Rowlinson S, Roy S, Roy S, Roy S, Rozza D, Ruggi P, Ryan K, Sachdev S, Sadecki T, Sadiq J, Bitossi M, Sago N, Saito S, Saito Y, Sakai K, Sakai Y, Sakellariadou M, Sakuno Y, Salafia O, Salconi L, Saleem M, Bizouard MA, Salemi F, Samajdar A, Sanchez E, Sanchez J, Sanchez L, Sanchis-Gual N, Sanders J, Sanuy A, Saravanan T, Sarin N, Blackburn J, Sassolas B, Satari H, Sathyaprakash B, Sato S, Sato T, Sauter O, Savage R, Sawada T, Sawant D, Sawant H, Blair C, Sayah S, Schaetzl D, Scheel M, Scheuer J, Schiworski M, Schmidt P, Schmidt S, Schnabel R, Schneewind M, Schofield R, Blair D, Schönbeck A, Schulte B, Schutz B, Schwartz E, Scott J, Scott S, Seglar-Arroyo M, Sekiguchi T, Sekiguchi Y, Sellers D, Blair R, Sengupta A, Sentenac D, Seo E, Sequino V, Sergeev A, Setyawati Y, Shaffer T, Shahriar M, Shams B, Shao L, Bobba F, Sharma A, Sharma P, Shawhan P, Shcheblanov N, Shibagaki S, Shikauchi M, Shimizu R, Shimoda T, Shimode K, Shinkai H, Bode N, Shishido T, Shoda A, Shoemaker D, Shoemaker D, ShyamSundar S, Sieniawska 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Subrahmanya SC, Champion E, Chan CH, Chan C, Chan C, Chan K, Chan M, Chandra K, Chanial P, Chao S, Charlton P, Chase E, Chassande-Mottin E, Chatterjee C, Chatterjee D, Chatterjee D, Chaturvedi M, Chaty S, Chen C, Chen H, Chen J, Chen K, Chen X, Chen YB, Chen YR, Chen Z, Cheng H, Cheong C, Cheung H, Chia H, Chiadini F, Chiang CY, Chiarini G, Chierici R, Chincarini A, Chiofalo M, Chiummo A, Cho G, Cho H, Choudhary R, Choudhary S, Christensen N, Chu H, Chu Q, Chu YK, Chua S, Chung K, Ciani G, Ciecielag P, Cieślar M, Cifaldi M, Ciobanu A, Ciolfi R, Cipriano F, Cirone A, Clara F, Clark E, Clark J, Clarke L, Clearwater P, Clesse S, Cleva F, Coccia E, Codazzo E, Cohadon PF, Cohen D, Cohen L, Colleoni M, Collette C, Colombo A, Colpi M, Compton C, Constancio M, Conti L, Cooper S, Corban P, Corbitt T, Cordero-Carrión I, Corezzi S, Corley K, Cornish N, Corre D, Corsi A, Cortese S, Costa C, Cotesta R, Coughlin M, Coulon JP, Countryman S, Cousins B, Couvares P, Coward D, Cowart M, Coyne D, Coyne R, Creighton J, Creighton T, Criswell A, Croquette M, Crowder S, Cudell J, Cullen T, Cumming A, Cummings R, Cunningham L, Cuoco E, Curyło M, Dabadie P, Canton TD, Dall’Osso S, Dálya G, Dana A, DaneshgaranBajastani L, D’Angelo B, Danilishin S, D’Antonio S, Danzmann K, Darsow-Fromm C, Dasgupta A, Datrier L, Datta S, Dattilo V, Dave I, Davier M, Davies G, Davis D, Davis M, Daw E, Dean R, DeBra D, Deenadayalan M, Degallaix J, De Laurentis M, Deléglise S, Del Favero V, De Lillo F, De Lillo N, Del Pozzo W, DeMarchi L, De Matteis F, D’Emilio V, Demos N, Dent T, Depasse A, De Pietri R, De Rosa R, De Rossi C, DeSalvo R, De Simone R, Dhurandhar S, Díaz M, Diaz-Ortiz M, Didio N, Dietrich T, Di Fiore L, Di Fronzo C, Di Giorgio C, Di Giovanni F, Di Giovanni M, Di Girolamo T, Di Lieto A, Ding B, Di Pace S, Di Palma I, Di Renzo F, Divakarla A, Dmitriev A, Doctor Z, D’Onofrio L, Donovan F, Dooley K, Doravari S, Dorrington I, Drago M, Driggers J, Drori Y, Ducoin JG, Dupej P, Durante O, D’Urso D, Duverne PA, Dwyer S, Eassa C, Easter P, Ebersold M, Eckhardt T, Eddolls G, Edelman B, Edo T, Edy O, Effler A, Eguchi S, Eichholz J, Eikenberry S, Eisenmann M, Eisenstein R, Ejlli A, Engelby E, Enomoto Y, Errico L, Essick R, Estellés H, Estevez D, Etienne Z, Etzel T, Evans M, Evans T, Ewing B, Fafone V, Fair H, Fairhurst S, Farah A, Farinon S, Farr B, Farr W, Farrow N, Fauchon-Jones E, Favaro G, Favata M, Fays M, Fazio M, Feicht J, Fejer M, Fenyvesi E, Ferguson D, Fernandez-Galiana A, Ferrante I, Ferreira T, Fidecaro F, Figura P, Fiori I, Fishbach M, Fisher R, Fittipaldi R, Fiumara V, Flaminio R, Floden E, Fong H, Font J, Fornal B, Forsyth P, Franke A, Frasca S, Frasconi F, Frederick C, Freed J, Frei Z, Freise A, Frey R, Fritschel P, Frolov V, Fronzé G, Fujii Y, Fujikawa Y, Fukunaga M, Fukushima M, Fulda P, Fyffe M, Gabbard H, Gadre B, Gair J, Gais J, Galaudage S, Gamba R, Ganapathy D, Ganguly A, Gao D, Gaonkar S, Garaventa B, García-Núñez C, García-Quirós C, Garufi F, Gateley B, Gaudio S, Gayathri V, Ge GG, Gemme G, Gennai A, George J, Gerberding O, Gergely L, Gewecke P, Ghonge S, Ghosh A, Ghosh A, Ghosh S, Ghosh S, Giacomazzo B, Giacoppo L, Giaime J, Giardina K, Gibson D, Gier C, Giesler M, Giri P, Gissi F, Glanzer J, Gleckl A, Godwin P, Goetz E, Goetz R, Gohlke N, Goncharov B, González G, Gopakumar A, Gosselin M, Gouaty R, Gould D, Grace B, Grado A, Granata M, Granata V, Grant A, Gras S, Grassia P, Gray C, Gray R, Greco G, Green A, Green R, Gretarsson A, Gretarsson E, Griffith D, Griffiths W, Griggs H, Grignani G, Grimaldi A, Grimm S, Grote H, Grunewald S, Gruning P, Guerra D, Guidi G, Guimaraes A, Guixé G, Gulati H, Guo HK, Guo Y, Gupta A, Gupta A, Gupta P, Gustafson E, Gustafson R, Guzman F, Ha S, Haegel L, Hagiwara A, Haino S, Halim O, Hall E, Hamilton E, Hammond G, Han WB, Haney M, Hanks J, Hanna C, Hannam M, Hannuksela O, Hansen H, Hansen T, Hanson J, Harder T, Hardwick T, Haris K, Harms J, Harry G, Harry I, Hartwig D, Hasegawa K, Haskell B, Hasskew R, Haster CJ, Hattori K, Haughian K, Hayakawa H, Hayama K, Hayes F, Healy J, Heidmann A, Heidt A, Heintze M, Heinze J, Heinzel J, Heitmann H, Hellman F, Hello P, Helmling-Cornell A, Hemming G, Hendry M, Heng I, Hennes E, Hennig J, Hennig M, Hernandez A, Vivanco FH, Heurs M, Hild S, Hill P, Himemoto Y, Hines A, Hiranuma Y, Hirata N, Hirose E, Hochheim S, Hofman D, Hohmann J, Holcomb D, Holland N, Hollows I, Holmes Z, Holt K, Holz D, Hong Z, Hopkins P, Hough J, Hourihane S, Howell E, Hoy C, Hoyland D, Hreibi A, Hsieh BH, Hsu Y, Huang GZ, Huang HY, Huang P, Huang YC, Huang YJ, Huang Y, Hübner M, Huddart A, Hughey B, Hui D, Hui V, Husa S, Huttner S, Huxford R, Huynh-Dinh T, Ide S, Idzkowski B, Iess A, Ikenoue B, Imam S, Inayoshi K, Ingram C, Inoue Y, Ioka K, Isi M, Isleif K, Ito K, Itoh Y, Iyer B, Izumi K, JaberianHamedan V, Jacqmin T, Jadhav S, Jadhav S, James A, Jan A, Jani K, Janquart J, Janssens K, Janthalur N, Jaranowski P, Jariwala D, Jaume R, Jenkins A, Jenner K, Jeon C, Jeunon M, Jia W, Jin HB, Johns G, Jones A, Jones D, Jones J, Jones P, Jones R, Jonker R, Ju L, Jung P, Jung K, Junker J, Juste V, Kaihotsu K, Kajita T, Kakizaki M, Kalaghatgi C, Kalogera V, Kamai B, Kamiizumi M, Kanda N, Kandhasamy S, Kang G, Kanner J, Kao Y, Kapadia S, Kapasi D, Karat S, Karathanasis C, Karki S, Kashyap R, Kasprzack M, Kastaun W, Katsanevas S, Katsavounidis E, Katzman W, Kaur T, Kawabe K, Kawaguchi K, Kawai N, Kawasaki T, Kéfélian F, Keitel D, Key J, Khadka S, Khalili F, Khan S, Khazanov E, Khetan N, Khursheed M, Kijbunchoo N, Kim C, Kim J, Kim J, Kim K, Kim W, Kim YM, Kimball C, Kimura N, Kinley-Hanlon M, Kirchhoff R, Kissel J, Kita N, Kitazawa H, Kleybolte L, Klimenko S, Knee A, Knowles T, Knyazev E, Koch P, Koekoek G, Kojima Y, Kokeyama K, Koley S, Kolitsidou P, Kolstein M, Komori K, Kondrashov V, Kong A, Kontos A, Koper N, Korobko M, Kotake K, Kovalam M, Kozak D, Kozakai C, Kozu R, Kringel V, Krishnendu N, Królak A, Kuehn G, Kuei F, Kuijer P, Kumar A, Kumar P, Kumar R, Kumar R, Kume J, Kuns K, Kuo C, Kuo HS, Kuromiya Y, Kuroyanagi S, Kusayanagi K, Kuwahara S, Kwak K, Lagabbe P, Laghi D, Lalande E, Lam T, Lamberts A, Landry M, Lane B, Lang R, Lange J, Lantz B, La Rosa I, Lartaux-Vollard A, Lasky P, Laxen M, Lazzarini A, Lazzaro C, Leaci P, Leavey S, Lecoeuche Y, Lee H, Lee H, Lee H, Lee J, Lee K, Lee R, Lehmann J, Lemaître A, Leonardi M, Leroy N, Letendre N, Levesque C, Levin Y, Leviton J, Leyde K, Li A, Li B, Li J, Li K, Li T, Li X, Lin CY, Lin FK, Lin FL, Lin H, Lin LCC, Linde F, Linker S, Linley J, Littenberg T, Liu G, Liu J, Liu K, Liu X, Llamas F, Llorens-Monteagudo M, Lo R, Lockwood A, London L, Longo A, Lopez D, Portilla ML, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lott T, Lough J, Lousto C, Lovelace G, Lucaccioni J, Lück H, Lumaca D, Lundgren A, Luo LW, Lynam J, Macas R, MacInnis M, Macleod D, MacMillan I, Macquet A, Hernandez IM, Magazzù C, Magee R, Maggiore R, Magnozzi M, Mahesh S, Majorana E, Makarem C, Maksimovic I, Maliakal S, Malik A, Man N, Mandic V, Mangano V, Mango J, Mansell G, Manske M, Mantovani M, Mapelli M, Marchesoni F, Marchio M, Marion F, Mark Z, Márka S, Márka Z, Markakis C, Markosyan A, Markowitz A, Maros E, Marquina A, Marsat S, Martelli F, Martin I, Martin R, Martinez M, Martinez V, Martinez V, Martinovic K, Martynov D, Marx E, Masalehdan H, Mason K, Massera E, Masserot A, Massinger T, Masso-Reid M, Mastrogiovanni S, Matas A, Mateu-Lucena M, Matichard F, Matiushechkina M, Mavalvala N, McCann J, McCarthy R, McClelland D, McClincy P, McCormick S, McCuller L, McGhee G, McGuire S, McIsaac C, McIver J, McRae T, McWilliams S, Meacher D, Mehmet M, Mehta A, Meijer Q, Melatos A, Melchor D, Mendell G, Menendez-Vazquez A, Menoni C, Mercer R, Mereni L, Merfeld K, Merilh E, Merritt J, Merzougui M, Meshkov S, Messenger C, Messick C, Meyers P, Meylahn F, Mhaske A, Miani A, Miao H, Michaloliakos I, Michel C, Michimura Y, Middleton H, Milano L, Miller A, Miller A, Miller B, Millhouse M, Mills J, Milotti E, Minazzoli O, Minenkov Y, Mio N, Mir L, Miravet-Tenés M, Mishra C, Mishra T, Mistry T, Mitra S, Mitrofanov V, Mitselmakher G, Mittleman R, Miyakawa O, Miyamoto A, Miyazaki Y, Miyo K, Miyoki S, Mo G, Moguel E, Mogushi K, Mohapatra S, Mohite S, Molina I, Molina-Ruiz M, Mondin M, Montani M, Moore C, Moraru D, Morawski F, More A, Moreno C. All-sky, all-frequency directional search for persistent gravitational waves from Advanced LIGO’s and Advanced Virgo’s first three observing runs. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.122001] [Citation(s) in RCA: 2] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Zhang HL, Wang ML, Yi LZ, Högger P, Arroo R, Bajpai VK, Prieto MA, Chen XJ, Simal-Gandara J, Cao H. Stability profiling and degradation products of dihydromyricetin in Dulbecco's modified eagle's medium. Food Chem 2022; 378:132033. [PMID: 35033717 DOI: 10.1016/j.foodchem.2021.132033] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/08/2021] [Revised: 12/20/2021] [Accepted: 12/31/2021] [Indexed: 11/30/2022]
Abstract
Dihydromyricetin has shown many bioactivities in cell level. However, dihydromyricetin was found to be highly instable in cell culture medium DMEM. Here, the underlying degradation mechanism was investigated via UPLC-MS/MS analysis. Dihydromyricetin was mainly converted into its dimers and oxidized products. At lower temperature, dihydromyricetin in DMEM showed higher stability. Vitamin C increased the stability of dihydromyricetin in DMEM probably due to its high antioxidant potential.
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Affiliation(s)
- H L Zhang
- Institute of Chinese Medical Sciences, University of Macau, Macao, China.
| | - M L Wang
- Institute of Chinese Medical Sciences, University of Macau, Macao, China.
| | - L Z Yi
- Faculty of Agriculture and Food, Kunming University of Science and Technology, Kunming, Yunnan 650500, China.
| | - P Högger
- Institut für Pharmazie und Lebensmittelchemie, Universität Würzburg, 97074 Würzburg, Germany.
| | - R Arroo
- De Montfort University - Leicester School of Pharmacy, The Gateway, Leicester LE1 9BH, UK.
| | - V K Bajpai
- Department of Energy and Materials Engineering, Dongguk University-Seoul, 30 Pildong-ro 1-gil, Seoul 04620, Republic of Korea
| | - M A Prieto
- Department of Analytical Chemistry and Food Science, Faculty of Food Science and Technology, University of Vigo - Ourense Campus, E-32004 Ourense, Spain.
| | - X J Chen
- Institute of Chinese Medical Sciences, University of Macau, Macao, China.
| | - J Simal-Gandara
- Department of Analytical Chemistry and Food Science, Faculty of Food Science and Technology, University of Vigo - Ourense Campus, E-32004 Ourense, Spain.
| | - H Cao
- Department of Analytical Chemistry and Food Science, Faculty of Food Science and Technology, University of Vigo - Ourense Campus, E-32004 Ourense, Spain; College of Food Science and Technology, Guangdong Ocean University, Zhanjiang 524088, China
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Alnuwaiser MA, Javaid K, Jacob J, Saleem M, Liang L, Cao H, Amami M, Mahmood K, Ali A, Amin N, Ikram S. Annealing induced morphology evolution and phase transition in SnOx thin films grown by e-beam evaporation method. INORG CHEM COMMUN 2022. [DOI: 10.1016/j.inoche.2022.109473] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/05/2022]
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Jin C, Liu W, Xu Y, Huang Y, Nie Y, Shi X, Zhang G, He P, Zhang J, Cao H, Sun J, Yang J. Artificial Vision Adaption Mimicked by an Optoelectrical In 2O 3 Transistor Array. Nano Lett 2022; 22:3372-3379. [PMID: 35343229 DOI: 10.1021/acs.nanolett.2c00599] [Citation(s) in RCA: 16] [Impact Index Per Article: 8.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
Simulation of biological visual perception has gained considerable attention. In this paper, an optoelectrical In2O3 transistor array with a negative photoconductivity behavior is designed using a side-gate structure and a screen-printed ion-gel as the gate insulator. This paper is the first to observe a negative photoconductivity in electrolyte-gated oxide devices. Furthermore, an artificial visual perception system capable of self-adapting to environmental lightness is mimicked using the proposed device array. The transistor device array shows a self-adaptive behavior of light under different levels of light intensity, successfully demonstrating the visual adaption with an adjustable threshold range to the external environment. This study provides a new way to create an environmentally adaptive artificial visual perception system and has far-reaching significance for the future of neuromorphic electronics.
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Affiliation(s)
- Chenxing Jin
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Wanrong Liu
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Yunchao Xu
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Yulong Huang
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Yiling Nie
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Xiaofang Shi
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Gengming Zhang
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Pei He
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Jian Zhang
- School of Material Science and Engineering, Guilin University of Electronic Technology, Guilin, 541004, P. R. China
| | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, P. R. China
| | - Jia Sun
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
| | - Junliang Yang
- Hunan Key Laboratory for Super Microstructure and Ultrafast Process, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China
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Wang J, Meng W, Yang J, Cao H, Liu T, Yang C, Yu M, Wang B. Aberrant methylation-mediated downregulation of the LINC01554 gene accelerates the malignant progression and regulates the chemosensitivity of laryngeal squamous cell carcinoma. J Physiol Pharmacol 2022; 73. [PMID: 35988928 DOI: 10.26402/jpp.2022.2.03] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Received: 01/21/2022] [Accepted: 04/30/2022] [Indexed: 06/15/2023]
Abstract
Laryngeal squamous cell carcinoma (LSCC) is diagnosed as a malignant tumor with a poor prognosis, the associated mechanisms still need to be further investigated. The LINC01554 gene is confirmed to participate in the tumorigenesis of hepatocellular carcinoma, but its role in LSCC has not been investigated. The aim of this study was to investigate the function and the potential mechanism of LINC01554 in LSCC, LINC01554 further was used as a molecular target for the diagnosis and molecular targeted therapy of LSCC. The microarray-based gene expression profiling of LSCC and its adjacent non-tumor tissue were used to identify the differentially expressed long non-coding RNAs (lncRNAs). Reverse transcription-quantitative polymerase chain reaction (RT-qPCR) was applied to verify the expression levels of LINC01554 in tissue and LSCC cell lines. The DNA methylation level of the LINC01554 promoter was detected by the application of bisulfite genomic sequencing (BGS), and the bisulfite conversion-specific/methylation-specific polymerase chain reaction (BS-MSP) method. The effect of LINC01554 on the proliferation, migration, and invasion of squamous cell carcinoma was assessed by MTS, wound healing, transwell, RT-qPCR, Western blot in vitro-cultured TU177 cells, and AMC-HN-8 cells. The microarray-based gene expression profiling identified the differentially expressed lncRNAs, including LINC01554, with downregulation in the LSCC tissue vs. normal tissue. The RT-qPCR verified the downregulation of LINC01554 in the LSCC tissue (P=0.0049) and LSCC cell (P=0.0020). The BGS and BS-MSP exhibited the hypermethylation level of the LINC01554 promoter, which mediated the downregulation of LINC01554. A gain-of-function experiment showed that LINC01554 inhibited the proliferation, migration, and invasion of TU177 and AMC-HN-8. Subsequently, LINC01554 overexpression was shown to decrease cell viability in TU177 and AMC-HN-8 cells treated with cisplatin. Our findings indicated that the aberrant methylation-mediated downregulation of LINC01554 promoted malignant progression and cisplatin resistance in LSCC, and LINC01554 may serve as a potential diagnostic biomarker and a novel therapeutic target for LSCC.
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Affiliation(s)
- J Wang
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - W Meng
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - J Yang
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - H Cao
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - T Liu
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - C Yang
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - M Yu
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China
| | - B Wang
- Department of Otorhinolaryngology, The Second Hospital of Hebei Medical University, Shijiazhuang, Hebei, China.
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Yu J, Gao G, Sun B, Liang L, Shen Q, Zhang Y, Cao H. Optimization of sensing-pad functionalizing strategy toward separative extended-gate FET biosensors for PSA detection. J Pharm Biomed Anal 2022; 211:114597. [DOI: 10.1016/j.jpba.2022.114597] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/18/2021] [Revised: 01/06/2022] [Accepted: 01/13/2022] [Indexed: 11/28/2022]
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Zhao EH, Cao H. [Current status and progression of minimally invasive surgery after neoadjuvant therapy for adenocarcinoma of esophagogastric junction]. Zhonghua Wei Chang Wai Ke Za Zhi 2022; 25:141-146. [PMID: 35176826 DOI: 10.3760/cma.j.cn441530-20211221-00523] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
The number of minimally invasive surgery (MIS) for adenocarcinoma of esophagogastric junction (AEG) has been increasing year by year. The key technical points such as surgical approach, lymph node dissection and GI tract reconstruction have gradually reached their maturity. With the emergence of proofs of evidence-based neoadjuvant therapy, neoadjuvant chemotherapy or neoadjuvant radiochemotherapy for advanced AEG is also gradually accepted by most surgeons and oncologists. European scholars have previously started researches on MIS after neoadjuvant therapy for esophageal cancer and AEG. Domestic scholars also raise practical suggestions on the application of neoadjuvant therapy for AEG via the cooperation between gastrointestinal and thoracic surgeons, demonstrating the trend in standardization and individualization. But there is still no consent to the indication of MIS after neoadjuvant therapy. Furthermore, there is also a lack of the standardization of technical points for MIS, GI tract reconstruction, short- and long-term outcomes. Such associated problems have been the hot controversy and exploration in recent years. This article describes current progress of neoadjuvant therapy for AEG, current status of MIS after the neoadjuvant therapy in Europe, America, East Asia, including China, and related researches plus future prospects, hoping for better clinical outcomes.
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Affiliation(s)
- E H Zhao
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - H Cao
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
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Li Y, Yin K, Diao Y, Fang M, Yang J, Zhang J, Cao H, Liu X, Jiang J. A biopolymer-gated ionotronic junctionless oxide transistor array for spatiotemporal pain-perception emulation in nociceptor network. Nanoscale 2022; 14:2316-2326. [PMID: 35084010 DOI: 10.1039/d1nr07896h] [Citation(s) in RCA: 20] [Impact Index Per Article: 10.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
Capable of reflecting the location and intensity of external harmful stimuli, a nociceptor network is of great importance for receiving pain-perception information. However, the hardware-based implementation of a nociceptor network through the use of a transistor array remains a great challenge in the area of brain-inspired neuromorphic applications. Herein, a simple ionotronic junctionless oxide transistor array with pain-perception abilities is successfully realized due to a coplanar-gate proton-coupling effect in sodium alginate biopolymer electrolyte. Several important pain-perception characteristics of nociceptors are emulated, such as a pain threshold, the memory of prior injury, and sensitization behavior due to pathway alterations. In particular, a good graded pain-perception network system has been successfully established through coplanar capacitance and resistance. More importantly, clear polarity reversal of Lorentz-type spatiotemporal pain-perception emulation can be finally realized in our projection-dependent nociceptor network. This work may provide new avenues for bionic medical machines and humanoid robots based on these intriguing pain-perception abilities.
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Affiliation(s)
- Yanran Li
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
| | - Kai Yin
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
| | - Yu Diao
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
| | - Mei Fang
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
| | - Junliang Yang
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
| | - Jian Zhang
- School of Material Science and Engineering, Guilin University of Electronic Technology, Guilin, 541004, P. R. China
| | - Hongtao Cao
- Laboratory of Advanced Nano Materials and Devices, Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, P. R. China
| | - Xiaoliang Liu
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
| | - Jie Jiang
- Hunan Key Laboratory of Nanophotonics and Devices, School of Physics and Electronics, Central South University, 932 South Lushan Road, Changsha, Hunan 410083, P. R. China.
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Cao H, Wen X, Hong D, Li Y, Hong D. POS-688 FRAILTY RATE OF PERITONEAL DIALYSIS PATIENTS: A META-ANALYSIS. Kidney Int Rep 2022. [DOI: 10.1016/j.ekir.2022.01.722] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/19/2022] Open
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Cao H, Li Y, Chen L, Lu Z, You T, Wang X, Ji B. Tripartite motif-containing 54 promotes gastric cancer progression by upregulating K63-linked ubiquitination of filamin C. Asia Pac J Clin Oncol 2022; 18:669-677. [PMID: 35098666 DOI: 10.1111/ajco.13747] [Citation(s) in RCA: 2] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/16/2021] [Accepted: 12/04/2021] [Indexed: 12/12/2022]
Abstract
BACKGROUND Tripartite motif (TRIM) proteins have been proved to contribute to cancer progression, while whether tripartite motif-containing 54 (TRIM54) could functionally influence gastric cancer (GC) progression remains elusive. METHODS The expression level of TRIM54 and filamin C (FLNC) in GC was determined by Western blot and online database. Cell Counting Kit-8 (CCK-8) assay, colony formation assay and Ethylenediurea (EdU) staining were performed to explore the effects of TRIM54 on GC cell proliferation. Transwell assay and wound healing assay were applied to detect the influence of TRIM54 on GC cell migration and invasion. Bioinformatics analysis and Co-immunoprecipitation assay (Co-Ip), Ubiquitination assay and Half-life assay were involved to explore the regulatory mechanism of TRIM54 on FLNC. RESULTS TRIM54 was upregulated in GC tissues and cells, and a higher expression level of TRIM54 indicated a shorter overall survival of GC patients. The overexpression of TRIM54 significantly enhanced proliferation, migration, and invasion of GC cells, and inhibition of TRIM54 expression exerted reverse effects on GC cells. Mechanistically, TRIM54 was determined as a post-translational mediator of FLNC, and TRIM54 was co-immunoprecipitated with FLNC and degraded its protein level via K63-linked ubiquitination of FLNC. Notably, FLNC efficiently inhibited GC progression by TRIM54 overexpression. CONCLUSION Collectively, our findings suggested that the TRIM54/FLNC axis could be considered as a potential prognostic biomarker for GC.
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Affiliation(s)
- Hongtao Cao
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Southern Medical University, Guangzhou, China
| | - Ye Li
- Department of Radiotherapy, The Fifth People's Hospital of Qinghai Province, Xining, China
| | - Liang Chen
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Southern Medical University, Guangzhou, China
| | - Zhuocai Lu
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Southern Medical University, Guangzhou, China
| | - Tian You
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Southern Medical University, Guangzhou, China
| | - Xiaolong Wang
- Department of Gastrointestinal Surgery, Huadu District People's Hospital, Southern Medical University, Guangzhou, China
| | - Baoyan Ji
- Department of Oncology, Qinghai Provincial People's Hospital, Xining, China
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Qi ZF, Wen FY, Cao H, Zhang L. [Research progress of follow-up monitoring design in mega cohort]. Zhonghua Liu Xing Bing Xue Za Zhi 2022; 43:134-138. [PMID: 35130665 DOI: 10.3760/cma.j.cn112338-20210221-00132] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 06/14/2023]
Abstract
With the increasing demand to study the cause of complex diseases, mega cohort has gradually replaced the traditional small sample cohort and become the hotspot of epidemiological research. Follow-up is the essential step in a cohort study to obtain the information about the onset and death of diseases, migration or loss of follow-up of the cases. Its quality has a direct impact on the conclusions of cohort study. Therefore, it is necessary to develop a reasonable follow-up monitoring program for a mega cohort.In this paper, we summarized the contents and methods of the follow-up monitoring program in the mega cohorts at home and abroad, which aimed to provide suggestions for the new cohort and improve the follow-up program for the existing cohort.
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Affiliation(s)
- Z F Qi
- Department of Epidemiology and Health Statistics, School of Public Health, Capital Medical University/Beijing Municipal Key Laboratory of Clinical Epidemiology, Beijing 100069, China
| | - F Y Wen
- Department of Epidemiology and Health Statistics, School of Public Health, Capital Medical University/Beijing Municipal Key Laboratory of Clinical Epidemiology, Beijing 100069, China
| | - H Cao
- Department of Epidemiology and Health Statistics, School of Public Health, Capital Medical University/Beijing Municipal Key Laboratory of Clinical Epidemiology, Beijing 100069, China
| | - L Zhang
- Department of Epidemiology and Health Statistics, School of Public Health, Capital Medical University/Beijing Municipal Key Laboratory of Clinical Epidemiology, Beijing 100069, China
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49
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Cao H, Hou P, Cao Q, Li Y, Wang S, Xie L. Exciplex Emission and Property Investigation Based on Cyano-substituted 9-Phenylfluorene Derivative. Acta Chimica Sinica 2022. [DOI: 10.6023/a22070335] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/12/2022]
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50
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Zhang R, Li X, Meng F, Bi J, Zhang S, Peng S, Sun J, Wang X, Wu L, Duan J, Cao H, Zhang Q, Gu L, Huang LF, Cao Y. Wafer-Scale Epitaxy of Flexible Nitride Films with Superior Plasmonic and Superconducting Performance. ACS Appl Mater Interfaces 2021; 13:60182-60191. [PMID: 34881876 DOI: 10.1021/acsami.1c18278] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/13/2023]
Abstract
Transition-metal nitrides (e.g., TiN, ZrN, TaN) are incredible materials with excellent complementary metal-oxide semiconductor compatibility and remarkable performance in refractory plasmonics and superconducting quantum electronics. Epitaxial growth of flexible transition-metal nitride films, especially at the wafer scale, is fundamentally important for developing high-performance flexible photonics and superconducting electronics, but the study is rare thus far. This work reports the high-quality epitaxy of 2-in. titanium nitride (TiN) films on flexible fluorophlogopite-mica (F-mica) substrates via reactive magnetron sputtering. Combined measurements of spectroscopic ellipsometry and electrical transport reveal the superior plasmonic and superconducting performance of TiN/F-mica films owing to the high single crystallinity. More interestingly, the superconductivity of these flexible TiN films can be manipulated by the bending states, and enhanced superconducting critical temperature TC is observed in convex TiN films with in-plane tensile strain. Density functional theory calculations reveal that the strain can tune the electron-phonon interaction strength and the resultant superconductivity of TiN films. This study provides a promising route toward integrating scalable single-crystalline transition-metal nitride films with flexible electronics for high-performance plasmonics and superconducting electronics.
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Affiliation(s)
- Ruyi Zhang
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Xinyan Li
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Fanqi Meng
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Jiachang Bi
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Shunda Zhang
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Shaoqin Peng
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
| | - Jie Sun
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Xinming Wang
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Liang Wu
- Faculty of Materials Science and Engineering, Kunming University of Science and Technology, Kunming 650093, China
| | - Junxi Duan
- School of Physics, Beijing Institute of Technology, Beijing 100081, China
| | - Hongtao Cao
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Qinghua Zhang
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Lin Gu
- Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
| | - Liang-Feng Huang
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
| | - Yanwei Cao
- Ningbo Institute of Materials Technology and Engineering, Chinese Academy of Sciences, Ningbo 315201, China
- Center of Materials Science and Optoelectronics Engineering, University of Chinese Academy of Sciences, Beijing 100049, China
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