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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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2
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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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Chen W, Liao L, Huang Z, Lu Y, Lin Y, Pei Y, Yi S, Huang C, Cao H, Tan B. Corrigendum: Patchouli alcohol improved diarrhea-predominant irritable bowel syndrome by regulating excitatory neurotransmission in the myenteric plexus of rats. Front Pharmacol 2024; 15:1394753. [PMID: 38560352 PMCID: PMC10979391 DOI: 10.3389/fphar.2024.1394753] [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] [Received: 03/02/2024] [Accepted: 03/04/2024] [Indexed: 04/04/2024] Open
Abstract
[This corrects the article DOI: 10.3389/fphar.2022.943119.].
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Affiliation(s)
- Wanyu Chen
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Lu Liao
- Shenzhen Hospital of Shanghai University of Traditional Chinese Medicine, Guangzhou, China
| | - Zitong Huang
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Yulin Lu
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Yukang Lin
- College of Integrated Chinese and Western Medicine, Hunan University of Chinese Medicine, Changsha, Hunan, China
| | - Ying Pei
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Shulin Yi
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Chen Huang
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Hongying Cao
- School of Chinese Materia Medica, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Bo Tan
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
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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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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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Tao H, Luo L, Li Y, Zhao D, Cao H, Liao X. A risk-based approach for accurately delineating the extent of soil contamination: The role of additional sampling in transition zones. Sci Total Environ 2024; 908:168231. [PMID: 37923268 DOI: 10.1016/j.scitotenv.2023.168231] [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] [Received: 05/28/2023] [Revised: 10/11/2023] [Accepted: 10/28/2023] [Indexed: 11/07/2023]
Abstract
Accurate soil contamination delineation is crucial for deciding where remediation efforts are required. However, misjudgments, either in underestimating or overestimating contamination extents could incur different risks: underestimation may result in environmental risks, while overestimation may lead to financial risks. This study proposed an approach based on environmental and financial risks (loss risk) to improve the performance of contamination delineation. Additionally, the impact of additional sampling in the transition zones on the contamination delineation was evaluated. This approach was demonstrated in Hechi, southwest China, where the soil was polluted by arsenic and cadmium. Initially, geostatistical simulation and 512 initial soil sampling were utilized to generate two maps: the conditional coefficient of variation (CCV) and the conditional probability of exceeding a critical threshold (CPT). These two maps were integrated to quantify the uncertainty in identifying the transition zones, guiding additional sampling. Out of 189 candidate sampling sites, we selected 100 additional sites to address high uncertainty. Subsequently, the minimization risk principle was employed to delineate contamination boundaries. The results showed that contaminated areas in the initial phase were significantly underestimated. Additional sampling in the transition zones improved the performance of soil contamination delineation. The performance metrics of Recall and F1 score for arsenic exhibited a notable enhancement of 6 % and 7 %, respectively. As for cadmium, there was an enhancement with Recall and F1 scores increasing by 4 % and 7 %, respectively. Adding 100 extra samples reduced the financial risks of arsenic and cadmium by 13 % and 11 %, respectively. In comparison, the 100 additional samples reduced the environmental risks of arsenic and cadmium by 55 % and 72 %, respectively. The study demonstrates that combining CCV and CPT for additional sampling efficiently mitigates the risks of delineating contaminated areas, which could help better understand the boundaries and gradient of contamination.
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Affiliation(s)
- Huan Tao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
| | - Lingzhi Luo
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China; University of Chinese Academy of Sciences, Beijing 100049, China.
| | - You Li
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
| | - Dan Zhao
- Center for Environmental Risk and Damage Assessment, Chinese Academy for Environmental Planning, Beijing 100012, China.
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China; University of Chinese Academy of Sciences, Beijing 100049, China.
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
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Staplin N, Haynes R, Judge PK, Wanner C, Green JB, Emberson J, Preiss D, Mayne KJ, Ng SYA, Sammons E, Zhu D, Hill M, Stevens W, Wallendszus K, Brenner S, Cheung AK, Liu ZH, Li J, Hooi LS, Liu WJ, Kadowaki T, Nangaku M, Levin A, Cherney D, Maggioni AP, Pontremoli R, Deo R, Goto S, Rossello X, Tuttle KR, Steubl D, Petrini M, Seidi S, Landray MJ, Baigent C, Herrington WG, Abat S, Abd Rahman R, Abdul Cader R, Abdul Hafidz MI, Abdul Wahab MZ, Abdullah NK, Abdul-Samad T, Abe M, Abraham N, Acheampong S, Achiri P, Acosta JA, Adeleke A, Adell V, Adewuyi-Dalton R, Adnan N, Africano A, Agharazii M, Aguilar F, Aguilera A, Ahmad M, Ahmad MK, Ahmad NA, Ahmad NH, Ahmad NI, Ahmad Miswan N, Ahmad Rosdi H, Ahmed I, Ahmed S, Ahmed S, Aiello J, Aitken A, AitSadi R, Aker S, Akimoto S, Akinfolarin A, Akram S, Alberici F, Albert C, Aldrich L, Alegata M, Alexander L, Alfaress S, Alhadj Ali M, Ali A, Ali A, Alicic R, Aliu A, Almaraz R, Almasarwah R, Almeida J, Aloisi A, Al-Rabadi L, Alscher D, Alvarez P, Al-Zeer B, Amat M, Ambrose C, Ammar H, An Y, Andriaccio L, Ansu K, Apostolidi A, Arai N, Araki H, Araki S, Arbi A, Arechiga O, Armstrong S, Arnold T, Aronoff S, Arriaga W, Arroyo J, Arteaga D, Asahara S, Asai A, Asai N, Asano S, Asawa M, Asmee MF, Aucella F, Augustin M, Avery A, Awad A, Awang IY, Awazawa M, Axler A, Ayub W, Azhari Z, Baccaro R, Badin C, Bagwell B, Bahlmann-Kroll E, Bahtar AZ, Baigent C, Bains D, Bajaj H, Baker R, Baldini E, Banas B, Banerjee D, Banno S, Bansal S, Barberi S, Barnes S, Barnini C, Barot C, Barrett K, Barrios R, Bartolomei Mecatti B, Barton I, Barton J, Basily W, Bavanandan S, Baxter A, Becker L, Beddhu S, Beige J, Beigh S, Bell S, Benck U, Beneat A, Bennett A, Bennett D, Benyon S, Berdeprado J, Bergler T, Bergner A, Berry M, Bevilacqua M, Bhairoo J, Bhandari S, Bhandary N, Bhatt A, Bhattarai M, Bhavsar M, Bian W, Bianchini F, Bianco S, Bilous R, Bilton J, Bilucaglia D, Bird C, Birudaraju D, Biscoveanu M, Blake C, Bleakley N, Bocchicchia K, Bodine S, Bodington R, Boedecker S, Bolduc M, Bolton S, Bond C, Boreky F, Boren K, Bouchi R, Bough L, Bovan D, Bowler C, Bowman L, Brar N, Braun C, Breach A, Breitenfeldt M, Brenner S, Brettschneider B, Brewer A, Brewer G, Brindle V, Brioni E, Brown C, Brown H, Brown L, Brown R, Brown S, Browne D, Bruce K, Brueckmann M, Brunskill N, Bryant M, Brzoska M, Bu Y, Buckman C, Budoff M, Bullen M, Burke A, Burnette S, Burston C, Busch M, Bushnell J, Butler S, Büttner C, Byrne C, Caamano A, Cadorna J, Cafiero C, Cagle M, Cai J, Calabrese K, Calvi C, Camilleri B, Camp S, Campbell D, Campbell R, Cao H, Capelli I, Caple M, Caplin B, Cardone A, Carle J, Carnall V, Caroppo M, Carr S, Carraro G, Carson M, Casares P, Castillo C, Castro C, Caudill B, Cejka V, Ceseri M, Cham L, Chamberlain A, Chambers J, Chan CBT, Chan JYM, Chan YC, Chang E, Chang E, Chant T, Chavagnon T, Chellamuthu P, Chen F, Chen J, Chen P, Chen TM, Chen Y, Chen Y, Cheng C, Cheng H, Cheng MC, Cherney D, Cheung AK, Ching CH, Chitalia N, Choksi R, Chukwu C, Chung K, Cianciolo G, Cipressa L, Clark S, Clarke H, Clarke R, Clarke S, Cleveland B, Cole E, Coles H, Condurache L, Connor A, Convery K, Cooper A, Cooper N, Cooper Z, Cooperman L, Cosgrove L, Coutts P, Cowley A, Craik R, Cui G, Cummins T, Dahl N, Dai H, Dajani L, D'Amelio A, Damian E, Damianik K, Danel L, Daniels C, Daniels T, Darbeau S, Darius H, Dasgupta T, Davies J, Davies L, Davis A, Davis J, Davis L, Dayanandan R, Dayi S, Dayrell R, De Nicola L, Debnath S, Deeb W, Degenhardt S, DeGoursey K, Delaney M, Deo R, DeRaad R, Derebail V, Dev D, Devaux M, Dhall P, Dhillon G, Dienes J, Dobre M, Doctolero E, Dodds V, Domingo D, Donaldson D, Donaldson P, Donhauser C, Donley V, Dorestin S, Dorey S, Doulton T, Draganova D, Draxlbauer K, Driver F, Du H, Dube F, Duck T, Dugal T, Dugas J, Dukka H, Dumann H, Durham W, Dursch M, Dykas R, Easow R, Eckrich E, Eden G, Edmerson E, Edwards H, Ee LW, Eguchi J, Ehrl Y, Eichstadt K, Eid W, Eilerman B, Ejima Y, Eldon H, Ellam T, Elliott L, Ellison R, Emberson J, Epp R, Er A, Espino-Obrero M, Estcourt S, Estienne L, Evans G, Evans J, Evans S, Fabbri G, Fajardo-Moser M, Falcone C, Fani F, Faria-Shayler P, Farnia F, Farrugia D, Fechter M, Fellowes D, Feng F, Fernandez J, Ferraro P, Field A, Fikry S, Finch J, Finn H, Fioretto P, Fish R, Fleischer A, Fleming-Brown D, Fletcher L, Flora R, Foellinger C, Foligno N, Forest S, Forghani Z, Forsyth K, Fottrell-Gould D, Fox P, Frankel A, Fraser D, Frazier R, Frederick K, Freking N, French H, Froment A, Fuchs B, Fuessl L, Fujii H, Fujimoto A, Fujita A, Fujita K, Fujita Y, Fukagawa M, Fukao Y, Fukasawa A, Fuller T, Funayama T, Fung E, Furukawa M, Furukawa Y, Furusho M, Gabel S, Gaidu J, Gaiser S, Gallo K, Galloway C, Gambaro G, Gan CC, Gangemi C, Gao M, Garcia K, Garcia M, Garofalo C, Garrity M, Garza A, Gasko S, Gavrila M, Gebeyehu B, Geddes A, Gentile G, George A, George J, Gesualdo L, Ghalli F, Ghanem A, Ghate T, Ghavampour S, Ghazi A, Gherman A, Giebeln-Hudnell U, Gill B, Gillham 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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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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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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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Huang J, Li H, Zhang Y, Liu J, Cao H, Long Y. Excitatory purinergic and cholinergic expression changed in a partial bladder outlet obstruction-induced overactive bladder rat model. Sci Rep 2023; 13:18395. [PMID: 37884550 PMCID: PMC10603080 DOI: 10.1038/s41598-023-45014-5] [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] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/14/2023] [Accepted: 10/14/2023] [Indexed: 10/28/2023] Open
Abstract
Overactive bladder (OAB) is a common, long-term symptom complex with a high prevalence in women worldwide. OAB has caused a social burden, and effective treatments are urgently needed. However, the pathogenesis of OAB has yet to be elucidated. Model rats underwent bladder outlet obstruction surgery. In the 2nd, 3rd, and 4th weeks after surgery, metabolic cages were used to detect the 12 h urine volume of rats in the sham and model groups. The urodynamic parameters bladder leak point pressure (BPLL), maximum voiding pressure (MVP), residual volume (RV), maximum bladder capacity (MBC), bladder compliance (BC), voided efficiency (VE), and non-voiding contractions (NVCs) were also detected. Moreover, the contractile responses of isolated detrusor muscles to electrical and carbachol stimulation were examined at the abovementioned time points. At the 4th week after surgery, the bladders of both groups were obtained for hematoxylin-eosin (H&E) and Masson's trichrome staining. Real-time qPCR and Western blot were performed to quantify the expression of choline acetyltransferase (ChAT) and solute carrier family 17 member 9 (SLC17A9). At week 4, compared with the sham group, the 12 h urine volume of PBOO group increased significantly. The BLPP, MVP, VE, MBC, and NVCs increased significantly, and the VE was significantly reduced in 4-week PBOO group. The contractile responses of isolated detrusor muscles to electrical and carbachol stimulation significantly increased in 4-week PBOO group. In the 4-week PBOO group, the bladder wall and the ratio of bladder muscle to collagen within the bladder smooth muscle layer wall were significantly higher than those in the sham group. ChAT and SLC17A9 mRNA and protein expression in the OAB model rats significantly increased. At 4 weeks after PBOO, the OAB model was successfully established. The gene and protein expression levels of ChAT and SLC17A9 increased in the bladder of the OAB model, suggesting that OAB may be related to increased excitatory purinergic and cholinergic expression.
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Affiliation(s)
- Jingyi Huang
- Guangzhou University of Chinese Medicine, No.232 Outer Ring East Road, Higher Education Mega Center, Guangzhou, Guangdong, China
| | - Hongliang Li
- Guangzhou University of Chinese Medicine, No.232 Outer Ring East Road, Higher Education Mega Center, Guangzhou, Guangdong, China
| | - Yao Zhang
- Guangzhou University of Chinese Medicine, No.232 Outer Ring East Road, Higher Education Mega Center, Guangzhou, Guangdong, China
| | - Jiaye Liu
- Guangzhou University of Chinese Medicine, No.232 Outer Ring East Road, Higher Education Mega Center, Guangzhou, Guangdong, China
| | - Hongying Cao
- Guangzhou University of Chinese Medicine, No.232 Outer Ring East Road, Higher Education Mega Center, Guangzhou, Guangdong, China.
| | - Yongling Long
- Guangzhou University of Chinese Medicine, No.232 Outer Ring East Road, Higher Education Mega Center, Guangzhou, Guangdong, 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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Pei Y, Wang R, Chen W, Yi S, Huang C, Liang S, Cao H, Xu Y, Tan B. Impaired colonic motility in high-glycemic diet-induced diabetic mice is associated with disrupted gut microbiota and neuromuscular function. Endocr Connect 2023; 12:e230078. [PMID: 37399524 PMCID: PMC10448599 DOI: 10.1530/ec-23-0078] [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] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 03/08/2023] [Accepted: 06/30/2023] [Indexed: 07/05/2023]
Abstract
Background Similar to the high-fat diet (HFD), the high-glycemic diet (HGD) contributes to the development and progression of type 2 diabetes mellitus (T2DM). However, the effect of HGD on gastrointestinal motility in T2DM and its underlying mechanisms remain unclear. Methods Thirty C57BL/6J mice were randomly designated into the normal-feeding diet (NFD) group, HFD group, and HGD group. The plasma glucose, plasma insulin, and gastrointestinal motility were examined. Meanwhile, the tension of isolated colonic smooth muscle rings was calculated, and the gut microbiota was analyzed by 16s rDNA high-throughput sequencing. Result After 16 weeks of HGD feeding, obesity, hyperglycemia, insulin resistance, and constipation were observed in HGD mice. Autonomic contraction frequency of the colonic neuromuscular system and electrical field stimulation-induced contractions were reduced in HGD mice. On the contrary, neuronal nitric oxide synthase activity and neuromuscular relaxation were found to be enhanced. Finally, gut microbiota analysis revealed that Rhodospirillaceae abundance significantly increased at the family level in HGD mice. At the genus level, the abundance of Insolitispirillum increased remarkably, whereas Turicibacter abundance decreased significantly in HGD mice. Conclusion HGD induced constipation in obese diabetic mice, which we speculated that it may be related to neuromuscular dysmotility and intestinal microbiota dysbiosis.
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Affiliation(s)
- Ying Pei
- Research Centre of Basic Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Rui Wang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Wanyu Chen
- Research Centre of Basic Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Shulin Yi
- Research Centre of Basic Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Chen Huang
- Research Centre of Basic Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Shaochan Liang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Hongying Cao
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Yifei Xu
- Shenzhen Traditional Chinese Medicine Hospital, The Fourth Clinical Medical College of Guangzhou University of Chinese Medicine, Shenzhen, China
| | - Bo Tan
- Research Centre of Basic Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
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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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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 H, Zhu Y, Wang S, Zhao S, Nie Y, Ji C, Wang Q, Liao X, Cao H, Liu X. Spatial-vertical variations of energetic compounds and microbial community response in soils from an ammunition demolition site in China. Sci Total Environ 2023; 875:162553. [PMID: 36898332 DOI: 10.1016/j.scitotenv.2023.162553] [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] [Subscribe] [Scholar Register] [Received: 12/09/2022] [Revised: 02/21/2023] [Accepted: 02/25/2023] [Indexed: 06/18/2023]
Abstract
Ammunition-related activities have caused severe energetic compound (EC) contamination and pose serious risks to ecosystems. However, little is known regarding the spatial-vertical variations of ECs or their migration in soils at ammunition demolition sites. Although the toxic effect of some ECs to microorganisms have been reported through laboratory simulations, the responses of indigenous microbial communities to ammunition demolition activities are unclear. In this study, the spatial-vertical variations of ECs in 117 topsoil samples and three soil profiles from a typical ammunition demolition site in China were studied. Heavy contamination of ECs was concentrated in the top soils of the work platforms, and ECs were also detected in the surrounding area and nearby farmland. ECs showed different migration characteristics in the 0-100 cm soil layer of the different soil profiles. Demolition activities and surface runoff play critical roles in the spatial-vertical variations and migration of ECs. These findings suggest that ECs are able to migrate from the topsoil to the subsoil and from the core demolition area to further ecosystems. The work platforms exhibited lower microbial diversity and different microbiota compositions compared to the surrounding areas and farmlands. Using the random forest analysis, pH and 1,3,5-trinitrobenzene (TNB) were characterized as the most important factors affecting microbial diversity. Network analysis revealed that Desulfosporosinus was highly sensitive to ECs and may be a unique indicator of EC contamination. These findings provide key information in understanding EC migration characteristics in soils and the potential threats to indigenous soil microorganisms in ammunition demolition sites.
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Affiliation(s)
- Huijun Zhang
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China
| | - Yongbing Zhu
- State Key Laboratory of NBC Protection for Civilian, Beijing 102205, China
| | - Shiyu Wang
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China
| | - Sanping Zhao
- State Key Laboratory of NBC Protection for Civilian, Beijing 102205, China
| | - Yaguang Nie
- Information Materials and Intelligent Sensing Laboratory of Anhui Province, Institutes of Physical Science and Information Technology, Anhui University, Hefei 230601, China
| | - Chao Ji
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China
| | - Qing Wang
- State Key Laboratory of NBC Protection for Civilian, Beijing 102205, China
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China
| | - Xiaodong Liu
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China; CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China.
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Hou Y, Li Y, Tao H, Cao H, Liao X, Liu X. Three-dimensional distribution characteristics of multiple pollutants in the soil at a steelworks mega-site based on multi-source information. J Hazard Mater 2023; 448:130934. [PMID: 36860071 DOI: 10.1016/j.jhazmat.2023.130934] [Citation(s) in RCA: 5] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/30/2022] [Revised: 01/26/2023] [Accepted: 02/01/2023] [Indexed: 06/18/2023]
Abstract
Soil pollution at steelworks mega-sites has become a severe environmental issue worldwide. However, due to the complex production processes and hydrogeology, the soil pollution distribution at steelworks is still unclear. This study scientifically cognized the distribution characteristics of polycyclic aromatic hydrocarbons (PAHs), volatile organic compounds (VOCs), and heavy metals (HMs) at a steelworks mega-site based on multi-source information. Specifically, firstly, 3D distribution and spatial autocorrelation of pollutants were obtained by interpolation model and local indicators of spatial associations (LISA), respectively. Secondly, the characteristics of horizontal distribution, vertical distribution, and spatial autocorrelations of pollutants were identified by combining multi-source information such as production processes, soil layers, and properties of pollutants. Horizontal distribution showed that soil pollution in steelworks mainly occurred in the front end of the steel process chain. Over 47% of PAHs and VOCs pollution area were distributed in coking plants and over 69% of HMs in stockyards. Vertical distribution indicated that HMs, PAHs, and VOCs were enriched in the fill, silt, and clay layers, respectively. Spatial autocorrelation of pollutants was positively correlated with their mobility. This study clarified the soil pollution characteristics at steelworks mega-sites, which can support the investigation and remediation of steelworks mega-sites.
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Affiliation(s)
- Yixuan Hou
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China; Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - You Li
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - Huan Tao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
| | - Xiaodong Liu
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China; CAS Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, 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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20
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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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Luo J, Li Y, Cao H, Zhu Y, Liu X, Li H, Liao X. Variations of microbiota in three types of typical military contaminated sites: Diversities, structures, influence factors, and co-occurrence patterns. J Hazard Mater 2023; 443:130290. [PMID: 36335906 DOI: 10.1016/j.jhazmat.2022.130290] [Citation(s) in RCA: 7] [Impact Index Per Article: 7.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/22/2022] [Revised: 10/15/2022] [Accepted: 10/28/2022] [Indexed: 06/16/2023]
Abstract
Contamination with energetic compounds (ECs) is common in military sites and poses a great risk to the environment and human health. However, its effects on the soil bacterial communities remain unclear. This study assessed the variations of bacterial communities, co-occurrence patterns, and their influence factors in three types of typical military-contaminated sites (artillery range, military-industrial site, and ammunition destruction site). The results showed that the most polluted sites were ammunition destruction sites, followed by military-industrial sites, whereas pollution in the artillery ranges was minimal. The average concentrations of ECs including 2,4,6-trinitrotoluene (TNT), hexahydro-1,3,5-trinitro-1,3,5-triazine (RDX), and octahydro-1,3,5,7-tetranitro-1,3,5,7-tetrazocine (HMX) in the study sites ranged 120-1.67 × 105, 20-7.20 × 104, and 180-2.38 × 105 μg/kg, respectively. Bacterial diversity and community structure in military-industrial and ammunition destruction sites were significantly changed, but not in artillery ranges. TNT, pH, and soil moisture are the critical factors affecting bacterial communities in contaminated military sites. Co-occurrence network analysis indicated that the pressure of ECs affected bacterial interactions and microbiota function. Our findings provide new insights into the variations in bacterial communities in EC-contaminated military sites and references for the bioremediation of ECs.
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Affiliation(s)
- Junpeng Luo
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences (CAS), Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China; University of Chinese Academy of Sciences, Beijing 100049, China
| | - You Li
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences (CAS), Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences (CAS), Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - Yongbing Zhu
- State Key Laboratory of NBC Protection for Civilian, Beijing 102205, China
| | - Xiaodong Liu
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China
| | - Haonan Li
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences (CAS), Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China; University of Chinese Academy of Sciences, Beijing 100049, China
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences (CAS), Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
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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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He J, Gao J, Zhu H, Zhao Y, Zhang X, Wang X, Wan S, Cao H, Zhai L, Wang Y, Wang S. Effects of NBP on postoperative cognitive dysfunction in rats via Nrf 2/ARE pathway. Aging (Albany NY) 2023; 15:276-286. [PMID: 36626245 PMCID: PMC9876636 DOI: 10.18632/aging.204481] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/26/2022] [Accepted: 12/29/2022] [Indexed: 01/11/2023]
Abstract
OBJECTIVE Postoperative cognitive dysfunction (POCD) is a common postoperative disease that threatens patients' quality of life, especially elderly patients. With the popularity of anesthesia/surgery, POCD has received more attention worldwide. The objective of this research is to evaluate 3-n-Butylphthalide (NBP)'s protective effect on postoperative cognitive function in rats and its related mechanisms. METHODS Tibial fracture models of senile rats of POCD were established and divided into blank control group, solvent group, NBP group, Nrf 2 agonist group, and Nrf 2 inhibitor group. The changes in the cognitive abilities of rats were systematically evaluated by the Morris water maze test. After hematoxylin-eosin (HE) staining of the hippocampus, the morphological and structural changes of hippocampal neurons were observed by light microscopy. The expressions of apoptosis-related proteins were analyzed by immunohistochemistry and Western blot was used to detect the expressions of Nrf 2,HO-1,Mfn1,Mfn2,Drp1 proteins. Moreover, the changes in the morphology of mitochondria were observed by transmission electron microscopy. RESULTS Through the water maze test, we observed that the incidence of postoperative cognitive impairment in the NBP, agonist, and inhibitor groups was substantially lower as compared to the blank control group and solvent group (P < 0.05). The expressions of Nrf 2, HO-1, Mfn1, Mfn2, and Drp1 proteins in the NBP group were upregulated in comparison to the blank control group and the solvent group. The expressions of related proteins in the inhibitor group were substantially lower in comparison to the NBP group. CONCLUSIONS NBP can affect the postoperative cognitive function of rats by activating the Nrf 2/ARE signaling pathway.
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Affiliation(s)
- Jianshuai He
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Junqiong Gao
- Department of Anesthesiology, Weihai Municipal Hospital, Weihai, China
| | - He Zhu
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Yang Zhao
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Xiaotian Zhang
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Xiufang Wang
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Shengnan Wan
- Department of Thyroid Surgery, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Hongying Cao
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Lin Zhai
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
| | - Yuanyong Wang
- Department of Thoracic Surgery, Tangdu Hospital of Air Force Military Medical University, Xi’an, China
| | - Shilei Wang
- Department of Anesthesiology, The Affiliated Hospital of Qingdao University, Qingdao, China
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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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Chen W, Liao L, Huang Z, Lu Y, Lin Y, Pei Y, Yi S, Huang C, Cao H, Tan B. Patchouli alcohol improved diarrhea-predominant irritable bowel syndrome by regulating excitatory neurotransmission in the myenteric plexus of rats. Front Pharmacol 2022; 13:943119. [PMID: 36452228 PMCID: PMC9703083 DOI: 10.3389/fphar.2022.943119] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [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: 05/13/2022] [Accepted: 10/31/2022] [Indexed: 09/07/2023] Open
Abstract
Background and Purpose: Irritable bowel syndrome (IBS) is usually associated with chronic gastrointestinal disorders. Its most common subtype is accompanied with diarrhea (IBS-D). The enteric nervous system (ENS) modulates major gastrointestinal motility and functions whose aberration may induce IBS-D. The enteric neurons are susceptible to long-term neurotransmitter level alterations. The patchouli alcohol (PA), extracted from Pogostemonis Herba, has been reported to regulate neurotransmitter release in the ENS, while its effectiveness against IBS-D and the underlying mechanism remain unknown. Experimental Approach: In this study, we established an IBS-D model in rats through chronic restraint stress. We administered the rats with 5, 10, and 20 mg/kg of PA for intestinal and visceral examinations. The longitudinal muscle myenteric plexus (LMMP) neurons were further immunohistochemically stained for quantitative, morphological, and neurotransmitters analyses. Key Results: We found that PA decreased visceral sensitivity, diarrhea symptoms and intestinal transit in the IBS-D rats. Meanwhile, 10 and 20 mg/kg of PA significantly reduced the proportion of excitatory LMMP neurons in the distal colon, decreased the number of acetylcholine (Ach)- and substance P (SP)-positive neurons in the distal colon and restored the levels of Ach and SP in the IBS-D rats. Conclusion and Implications: These findings indicated that PA modulated LMMP excitatory neuron activities, improved intestinal motility and alleviated IBS-induced diarrheal symptoms, suggesting the potential therapeutic efficacy of PA against IBS-D.
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Affiliation(s)
- Wanyu Chen
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Lu Liao
- Shenzhen Hospital of Shanghai University of Traditional Chinese Medicine, Guangzhou, China
| | - Zitong Huang
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Yulin Lu
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Yukang Lin
- College of Integrated Chinese and Western Medicines, Hunan University of Chinese Medicine, Changsha, Hunan, China
| | - Ying Pei
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Shulin Yi
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Chen Huang
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Hongying Cao
- School of Chinese Materia Medica, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Bo Tan
- Research Centre of Basic Intergrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
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Chen Y, Yang Q, Xu J, Tang L, Zhang Y, Du F, Zhao Y, Wu X, Li M, Shen J, Ding R, Cao H, Li W, Li X, Chen M, Wu Z, Cho CH, Du Y, Wen Q, Xiao Z. PROTACs in Gastrointestinal Cancers. Molecular Therapy - Oncolytics 2022; 27:204-223. [DOI: 10.1016/j.omto.2022.10.012] [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: 11/06/2022]
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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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Li Y, Hou Y, Tao H, Cao H, Liu X, Wang Z, Liao X. An improved non-stationary geostatistical method for three-dimensional interpolation of Benzo(a)pyrene at a contaminated site. Sci Total Environ 2022; 838:156169. [PMID: 35613641 DOI: 10.1016/j.scitotenv.2022.156169] [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] [Subscribe] [Scholar Register] [Received: 03/24/2022] [Revised: 05/18/2022] [Accepted: 05/19/2022] [Indexed: 06/15/2023]
Abstract
Intense industrial activities and complex hydrogeological conditions at contaminated sites make accurate three-dimensional (3D) mapping challenging. The cause is the non-stationarity in the variance of soil pollutants in geographical space (G-space), making the stationary hypothesis required by the Kriging method unsatisfactory. To handle the variance non-stationarity, a Variance-Octree-Kriging (VOK) method was proposed. VOK is a spatial deformation method that constructs a stationary deformation space (D-space) by stretching and shrinking the G-spaces with low and high spatial correlation, respectively. VOK method consists of 3D stratification in G-space, space scaling and transformation, and ordinary Kriging (OK) in D-space. 3D stratification uses variance octree (VOT) to generate a set of anchor points in the G-space. The spatial scaling and transformation use the virtual force algorithm (VFA) and thin-plate spline to evenly distribute the anchor points and obtain the D-space, where the OK is implemented. The method was applied to predict the distribution of soil Benzo(a)pyrene (BaP) at a contaminated site in North China Plain. The results show that the interpolation accuracy of VOK was 9% higher than that of OK. The VOK method also changed the spatial structure from anisotropic to isotropic. The root mean squared error (RMSE) of fill, silt and clay layers decreased by 4.67%, 11.39%, and 20.46%, respectively. This method is applicable to the 3D interpolation of pollutants at contaminated sites, with the advantages of high interpolation accuracy and the ability to handle the non-stationarity in variance.
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Affiliation(s)
- You Li
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - Yixuan Hou
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China
| | - Huan Tao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China; University of Chinese Academy of Sciences, Beijing 100049, China
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China
| | - Xiaodong Liu
- School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui 230026, China
| | - Ziwei Wang
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China; University of Chinese Academy of Sciences, Beijing 100049, China
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing 100101, China; Beijing Key Laboratory of Environmental Damage Assessment and Remediation, Beijing 100101, China.
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Zhang Y, Zhang J, Hong M, Huang J, Xu S, Wang R, Zhou N, Huang P, Tan B, Cao H. Suo Quan Wan ameliorates bladder overactivity and regulates neurotransmission via regulating Myosin Va protein expression. Phytomedicine 2022; 104:154265. [PMID: 35763954 DOI: 10.1016/j.phymed.2022.154265] [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] [Subscribe] [Scholar Register] [Received: 12/02/2021] [Revised: 05/31/2022] [Accepted: 06/09/2022] [Indexed: 06/15/2023]
Abstract
BACKGROUND Ancient prescriptions of Suo Quan Wan (SQW) have therapeutic effects on diabetic bladder dysfunction. However, the underlying mechanism remains unclear. Here, we hypothesized that SQW ameliorates bladder overactivity and regulates neurotransmission via regulating Myosin Va protein expression. METHODS After diabetic rats were induced by streptozotocin (65 mg/kg), the model of diabetic bladder dysfunction was established by detecting fasting blood glucose, urodynamic test, in vitro muscle strip experiments, and histological examination. One week after induction, SQW was given to observe the therapeutic effect. The expression levels of Myosin Va in control, Model, SQW L and SQW H groups were detected by RT-qPCR, RNAscope and immunofluorescence assay. The expression levels of ChAT, SP, nNOS and VIP proteins were observed by immunofluorescence assay. After knockdown and overexpression of Myosin Va, the expression changes of ChAT, SP, nNOS and VIP and the regulatory role of SQW were observed. RESULTS STZ-induced DM rats had significantly higher serum glucose levels and lower body weight. Compared with the diabetic rats, SQW treatment significantly improved urination function with decreased residual volume (RV), bladder compliance (BC), non-voiding contractions (NVCs), and increased voided efficiency (VE). In addition, contractile responses of muscle strips to electrical-field stimulation (EFS), carbachol (CCh), KCl were significantly lower in the SQW H and SQW L groups than those in the model group. RT-qPCR found that the expression of Myosin Va in the bladder tissue or bladder neurons in model group was significantly increased compared with the control group, and SQW treatment significantly decreased the levels of Myosin Va. In DM rats, ChAT and SP expression were significantly increased, while nNOS and VIP expression were significantly decreased, and SQW improved this phenomenon. Interestingly, SQW ameliorated the abnormal expression of ChAT, SP, nNOS and VIP caused by myosin Va knockdown, and Myosin Va overexpression results are consistent with these. CONCLUSIONS SQW ameliorates overactive bladder and regulate neurotransmission via regulating Myosin Va mRNA and protein expression.
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Affiliation(s)
- Yao Zhang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Jiao Zhang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Ming Hong
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Jingyi Huang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Siyuan Xu
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Rui Wang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Na Zhou
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Ping Huang
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Bo Tan
- School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Hongying Cao
- School of Pharmaceutical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China.
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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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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, 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Washimi T, Washington N, Watchi J, Weaver B, Weaving C, Webster S, Weinert M, Weinstein A, Boschi V, Weiss R, Weller C, Weller R, Wellmann F, Wen L, Weßels P, Wette K, Whelan J, White D, Whiting B, Bose N, Whittle C, Wilken D, Williams D, Williams M, Williamson A, Willis J, Willke B, Wilson D, Wipf C, Wlodarczyk T, Bose S, Woan G, Woehler J, Wofford J, Wong D, Wong I, Wright M, Wu C, Wu D, Wu H, Wysocki D, Bossilkov V, Xiao L, Yamada T, Yamamoto H, Yamamoto K, Yamamoto T, Yamashita K, Yamazaki R, Yang F, Yang K, Yang L, Boudart V, Yang YC, Yang Y, Yang Y, Yap M, Yeeles D, Yeh SW, Yelikar A, Ying M, Yokoyama J, Yokozawa T, Bouffanais Y, Yoo J, Yoshioka T, Yu H, Yu H, Yuzurihara H, Zadrożny A, Zanolin M, Zeidler S, Zelenova T, Zendri JP, Bozzi A, Zevin M, Zhan M, Zhang H, Zhang J, Zhang L, Zhang R, Zhang T, Zhang Y, Zhao C, Zhao G, Bradaschia C, Zhao Y, Zhao Y, Zhou R, Zhou Z, Zhu X, Zhu ZH, Zucker M, Zweizig J, Brady P, Bramley A, Branch A, Branchesi M, Brau J, Breschi M, Briant T, Briggs J, Brillet A, Brinkmann M, Brockill P, Brooks A, Brooks J, Brown D, Brunett S, Bruno G, Bruntz R, Bryant J, Bucci F, Bulik T, Bulten H, Buonanno A, Burtnyk K, Buscicchio R, Buskulic D, Buy C, Byer R, Davies GC, Cabras G, Cabrita R, Cadonati L, Caesar M, Cagnoli G, Cahillane C, Bustillo JC, Callaghan J, Callister T, Calloni E, Cameron J, Camp J, Canepa M, Canevarolo S, Cannavacciuolo M, Cannon K, Cao H, Cao Z, Capocasa E, Capote E, Carapella G, Carbognani F, Carlassara M, Carlin J, Carney M, Carpinelli M, Carrillo G, Carullo G, Carver T, Diaz JC, Casentini C, Castaldi G, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Cella G, Cerdá-Durán P, Cesarini E, Chaibi W, Subrahmanya SC, Champion E, Chan CH, Chan C, Chan C, Chan K, Chan M, Chandra K, Chang I, Chanial P, Chao S, Chapman-Bird C, Charlton P, Chase E, Chassande-Mottin E, Chatterjee C, Chatterjee D, Chatterjee D, Chaturvedi M, Chaty S, Chen C, Chen D, Chen H, Chen J, Chen K, Chen X, Chen YB, Chen YR, Chen Z, Cheng H, Cheong C, 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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, Dell’Aquila D, 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, 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, Di Michele A, Ding B, Di Pace S, Di Palma I, Di Renzo F, Divakarla A, Dmitriev A, Doctor Z, Donahue L, D’Onofrio L, Donovan F, Dooley K, Doravari S, Drago M, Driggers J, Drori Y, Ducoin JG, Dupej P, Dupletsa U, 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, Evstafyeva T, Ewing B, Fabrizi F, Faedi F, Fafone V, Fair 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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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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, 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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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Cao H, Wang Z, Liao X, Li Y, Zhu Y. Research on the Regional Environmental Impact and Risk Assessment Affected by Mineral Resource Development: A Case Study of the Taojia River Watershed in Hunan. Front Ecol Evol 2022. [DOI: 10.3389/fevo.2022.918446] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
Abstract
The mining and production of mineral resources can directly lead to soil and water pollution, posing a serious threat to human health. In this study, the Taojia River basin, a tributary of the Xiangjiang River, was selected as the study area. Based on the concentrations of heavy metals (As, Cd, Pb, and Zn) in 653 soil/substrate samples collected from 342 points in the study area in 2013 and 2021, the changes in soil heavy metal concentrations in the region were systematically analyzed to assess their environmental risks and impacts on regional environmental quality. The results showed that from 2013 to 2021, the As, Pb, and Zn pollution in regional soil, tailing sand, and surface water was reduced, while the Cd pollution increased. The average soil As, Pb, and Zn concentrations decreased from 3,750, 2,340, and 1,180 mg/kg to 457, 373, and 387mg/kg, respectively, while the Cd concentration increased from 0.11to 1.91 mg/kg; additionally, the overall distribution trend of heavy metal concentrations was high in the south, low in the north, and gradually decreased from upstream to downstream. The single evaluation index of heavy metal pollution risk showed that the percentages of medium to heavy pollution points in the soil As, Pb, and Zn were 84, 57, and 28%, respectively, in 2013, and this index decreased to 38, 37, and 25%, respectively, in 2021. The regional environmental quality was closely related to the intensity of mineral resource development. From 2000 to 2010, frequent mining development activities led to an increase in the area of construction land and a continuous decrease in the area of arable land, grassland, and vegetation cover in the region. During 2010–2020, the area of construction land decreased, and the vegetation coverage increased. The comprehensive evaluation index showed that the overall soil pollution risk in the watershed decreased, and the proportion of heavily polluted points decreased from 80 to 65%. It was shown by principal component analysis and factor analysis that mining development activities were the largest source of heavy metal pollution, in addition to mixed sources of tailings, solid waste, agriculture, and traffic emission sources. The results provide a scientific basis for the management and risk control of heavy metal pollution in the Taojia River basin.
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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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Zhang H, Wang S, Zhu Y, Zhao S, Nie Y, Liao X, Cao H, Yin H, Liu X. Determination of Energetic Compounds in Ammunition Contaminated Soil by Accelerated Solvent Extraction (ASE) and Gas Chromatography – Microelectron Capture Detection (GC-µECD). ANAL LETT 2022. [DOI: 10.1080/00032719.2022.2059495] [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] [Indexed: 11/01/2022]
Affiliation(s)
- Huijun Zhang
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, China
| | - Shiyu Wang
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, China
| | - Yongbing Zhu
- State Key Laboratory of NBC Protection for Civilian, Beijing, China
| | - Sanping Zhao
- State Key Laboratory of NBC Protection for Civilian, Beijing, China
| | - Yaguang Nie
- Information Materials and Intelligent Sensing Laboratory of Anhui Province, Institutes of Physical Science and Information Technology, Anhui University, Hefei, China
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing, China
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing, China
| | - Hao Yin
- Instruments' Center for Physical Science, University of Science and Technology of China, Hefei, China
| | - Xiaodong Liu
- Anhui Province Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, 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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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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Zhang H, Zhu Y, Wang S, Zhao S, Nie Y, Liao X, Cao H, Yin H, Liu X. Contamination characteristics of energetic compounds in soils of two different types of military demolition range in China. Environ Pollut 2022; 295:118654. [PMID: 34890741 DOI: 10.1016/j.envpol.2021.118654] [Citation(s) in RCA: 4] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/13/2021] [Revised: 10/17/2021] [Accepted: 12/05/2021] [Indexed: 06/13/2023]
Abstract
The pollution of energetic compounds (ECs) in military ranges has become the focus of worldwide attention. However, few studies on the contamination of ECs at Chinese military ranges have been reported to date. In this study, two different types of military demolition range in China, Dunhua (DH) and Taiyuan (TY), were investigated and the ECs in their soils were determined. 10 ECs were detected at both ranges. While all the contamination characteristics were distinct, 2,4,6-trinitrotoluene (TNT) was the most abundant contamination source in soils at DH range, with an average concentration of 1106 mg kg-1 and a maximum concentration of 34,083 mg kg-1. Hexahydro-1,3,5-trinitro-1,3,5-triazine (RDX) and two mono-amino degradation products of TNT were also found to have high concentrations, with potential ecological and human health risks. In contrast, the concentrations of ECs in soils of TY range were much lower. The content of RDX was most significant, with average and maximum concentrations of 7.8 and 158 mg kg-1, respectively. However, the potential threat to human health of 2,4-dinitrotoluene and 2,6-dinitrotoluene in soils at both ranges should not be ignored. The differences in pollution characteristics of the ECs at DH and TY are closely related to the types and amounts of the munitions destroyed. Moreover, the spatial distribution of ECs at the demolition ranges was extremely heterogeneous, which may be attributed to the use of open burning / open detonation and the non-homogeneous composition of the munitions.
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Affiliation(s)
- Huijun Zhang
- Institute of Polar Environment & Anhui Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, 230026, China
| | - Yongbing Zhu
- State Key Laboratory of NBC Protection for Civilian, Beijing, 102205, China
| | - Shiyu Wang
- Institute of Polar Environment & Anhui Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, 230026, China
| | - Sanping Zhao
- State Key Laboratory of NBC Protection for Civilian, Beijing, 102205, China
| | - Yaguang Nie
- Information Materials and Intelligent Sensing Laboratory of Anhui Province, Institutes of Physical Science and Information Technology, Anhui University, Hefei, 230601, China
| | - Xiaoyong Liao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing, 100101, China
| | - Hongying Cao
- Key Laboratory of Land Surface Pattern and Simulation, Institute of Geographic Sciences and Natural Resources Research, Chinese Academy of Sciences, Beijing, 100101, China
| | - Hao Yin
- Instruments' Center for Physical Science, University of Science and Technology of China, Hefei, 230026, China
| | - Xiaodong Liu
- Institute of Polar Environment & Anhui Key Laboratory of Polar Environment and Global Change, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, 230026, China.
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41
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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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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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43
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Liu S, Zhang Y, Yang F, Gu J, Zhang R, Kuang Y, Mai W, Zheng C, Yu Y, Lu R, Zeng L, Cao H, Long Y. Modified Cangfu Daotan decoction ameliorates polycystic ovary syndrome with insulin resistance via NF-κB/LCN-2 signaling pathway in inflammatory microenvironment. Front Endocrinol (Lausanne) 2022; 13:975724. [PMID: 36440213 PMCID: PMC9686851 DOI: 10.3389/fendo.2022.975724] [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] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 06/28/2022] [Accepted: 10/20/2022] [Indexed: 11/09/2022] Open
Abstract
This study explored the possible connection between the insulin resistance-targeting protein adipokine lipocalin-2 (LCN-2) and NF-κB signaling pathway in the inflammatory microenvironment in PCOS-IR model rats to determine the pharmacological mechanism of modified Cangfu Daotan decoction (MCDD) intervention for PCOS-IR. We used a high-fat diet (42 days) combined with letrozole (1 mg/kg/day, 42 days) to establish a PCOS-IR rat model. From the third week after modeling, the rats were given continuous administration of MCDD (high dose with 31.68 g/kg, medium dose with 15.84 g/kg, and low dose with 7.92 g/kg) for 28 days. Serum, ovarian tissue, liver, and adipose tissue were collected after the last gavage. Enzyme-linked immunosorbent assay, hematoxylin-eosin (HE) staining, Masson staining, qRT-PCR, and Western blot experiments were performed to detect various indicators. Our results showed that MCDD could reduce body weight and abdominal fat weight; restore normal estrous cycle and ovarian function; alleviate fatty liver; regulate HOMA-IR and OGTT index; reduce serum inflammatory factor levels, LCN-2 level, and gene expression; and regulate the insulin signal transduction and NF-κB pathways in PCOS-IR rats. Thus, MCDD may play a role in improving ovarian function in PCOS-IR rats by downregulating NF-κB/LCN-2 proteins and upregulating the gene expression of Insr/Irs-1/Glut4 in the insulin signaling pathway in the inflammatory environment.
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Affiliation(s)
- Shuowen Liu
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Yao Zhang
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Fang Yang
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Jingna Gu
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Ruyue Zhang
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Yingying Kuang
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Wantong Mai
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Chengbo Zheng
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Yang Yu
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Ruling Lu
- Department of Gynecology, the First Affiliated Hospital of Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Lei Zeng
- Department of Gynecology, the First Affiliated Hospital of Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Hongying Cao
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
| | - Yongling Long
- School of Pharmaceutical Science, Guangzhou University of Chinese Medicine, Guangzhou, Guangdong, China
- *Correspondence: Yongling Long,
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Lin Q, Lun J, Zhang J, He X, Gong Z, Gao X, Cao H. [Gut microbiome composition in pre-adolescent children with different meat consumption patterns]. Nan Fang Yi Ke Da Xue Xue Bao 2021; 41:1801-1088. [PMID: 35012911 DOI: 10.12122/j.issn.1673-4254.2021.12.07] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 12/28/2022]
Abstract
OBJECTIVE To compare the composition of gut microbiome in pre-adolescent children with different meat consumption patterns. METHODS This study was conducted among 44 healthy school-age children (age range 8-10 years) in Shenzhen. According to the monthly intake frequency ratio of white meat and red meat, the children were divided into red-meat group (n=15), balanced group (n=16) and white-meat group (n=13). The Food Frequency Questionnaire (FFQ) was used to investigate the children's diet, and samples of morning feces were collected to study the gut microbiome. The fecal DNA was extracted and amplified, and the composition of the intestinal microbiome of the children was analyzed using Illumina Miseq high-throughput sequencing. RESULTS The children in red meat and white meat groups showed significantly lower abundance and diversity of gut microbiota than those with a balanced diet (P < 0.05). LEfSe analysis of the genus in the fecal samples showed that Escherichia-Shigella, Coprobacillus and Peptoniphilus were enriched in red-meat group and Holdemanella was enriched in the white-meat group as compared with the balanced group. In the samples of the balanced group, 31 and 25 genus (such as Laurespirillum and Rumenococcus) were significantly enriched as compared with the samples of the red-meat group and the white-meat group, respectively. Prediction of the gut microbiota KEGG pathway using PICRUSt2 suggested that compared with that in the balanced group, the gut microbiota in red-meat group had significant activation of the pathways involving lipopolysaccharide biosynthesis (P < 0.01), arachidonic acid metabolism (P < 0.01), thyroid hormone synthesis (P < 0.001), and carbohydrate digestion and absorption (P < 0.05). But compared with the white-meat group, the red-meat group showed only significant activation of the pathways of arachidonic acid metabolism (P < 0.05) and thyroid hormone synthesis (P < 0.05). CONCLUSION The preference of red meat and white meat consumption may significantly reduce the abundance and diversity of gut microbiota in pre-adolescent children. A red meat-rich diet may cause enrichment of Escherichia-Shigella and significant activation of lipopolysaccharide biosynthesis pathway, suggesting the potential benefit of a balanced diet for pre-adolescent children.
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Affiliation(s)
- Q Lin
- Department of Microbiology, Guangdong Provincial Key Laboratory of Tropical Diseases Research, School of Public Health, Southern Medical University, Guangzhou 510515, China
| | - J Lun
- Department of Microbiology, Guangdong Provincial Key Laboratory of Tropical Diseases Research, School of Public Health, Southern Medical University, Guangzhou 510515, China
| | - J Zhang
- Department of Rehabilitation Medicine, Nanfang Hospital, Southern Medical University, Guangzhou 510515, China
| | - X He
- Department of Microbiology, Guangdong Provincial Key Laboratory of Tropical Diseases Research, School of Public Health, Southern Medical University, Guangzhou 510515, China
| | - Z Gong
- Department of Microbiology, Guangdong Provincial Key Laboratory of Tropical Diseases Research, School of Public Health, Southern Medical University, Guangzhou 510515, China
| | - X Gao
- Department of Microbiology, Guangdong Provincial Key Laboratory of Tropical Diseases Research, School of Public Health, Southern Medical University, Guangzhou 510515, China
| | - H Cao
- Department of Microbiology, Guangdong Provincial Key Laboratory of Tropical Diseases Research, School of Public Health, Southern Medical University, Guangzhou 510515, China
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Ma L, He W, Li X, Liu X, Cao H, Guo L, Xiao X, Xu Y, Wu Y. Decreased CSF Dynamics in Treatment-Naive Patients with Essential Hypertension: A Study with Phase-Contrast Cine MR Imaging. AJNR Am J Neuroradiol 2021; 42:2146-2151. [PMID: 34620585 DOI: 10.3174/ajnr.a7284] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [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: 01/08/2021] [Accepted: 08/05/2021] [Indexed: 12/28/2022]
Abstract
BACKGROUND AND PURPOSE Arterial sclerosis resulting from hypertension slows CSF transportation in the perivascular spaces, showing the intrinsic relationship between the CSF and the blood vasculature. However, the exact effect of hypertension on human CSF flow dynamics remains unclear. The present study aimed to evaluate CSF flow dynamics in treatment-naive patients with essential hypertension using phase-contrast cine MR imaging. MATERIALS AND METHODS The study included 60 never-treated patients with essential hypertension and 60 subjects without symptomatic atherosclerosis. CSF flow parameters, such as forward flow volume, forward peak velocity, reverse flow volume, reverse peak velocity, average flow, and net flow volume, were measured with phase-contrast cine MR imaging. Differences between the 2 groups were assessed to determine the independent determinants of these CSF flow parameters. RESULTS Forward flow volume, forward peak velocity, reverse flow volume, reverse peak velocity, and average flow in the patients with hypertension significantly decreased (all, P < .05). Increasing systolic blood pressure was significantly associated with lower forward flow volume (β = -0.44 mL/mL/mm Hg; 95% CI, -0.83 to -0.06 mL/mL/mm Hg), forward peak velocity (β = -0.50 cm/s/mm Hg; 95% CI, -0.88 to -0.12 cm/s/mm Hg), reverse flow volume (β = -0.61 mL/mL/mm Hg; 95% CI, -0.97 to -0.26 mL/mL/mm Hg), reverse peak velocity (β = -0.55 cm/s/mm Hg; 95% CI, -0.91-0.18 cm/s/mm Hg), and average flow (β = -0.50 mL/min/mm Hg; 95% CI, -0.93 to -0.08 mL/min/mm Hg). CONCLUSIONS The CSF flow dynamics in patients with hypertension are decreased, and increasing systolic blood pressure is strongly associated with lower CSF flow dynamics.
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Affiliation(s)
- L Ma
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - W He
- Department of Radiology (W.H.), Guangdong 999 Brain Hospital, Guangzhou, China
| | - X Li
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - X Liu
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - H Cao
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - L Guo
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - X Xiao
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - Y Xu
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
| | - Y Wu
- From the Department of Medical Imaging (L.M., X. Li, X. Liu, H.C., L.G., X.X., Y.X., Y.W.), Nanfang Hospital, Southern Medical University, Guangzhou, China
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Abstract
Tooth extraction is one of the most common causes of dental anxiety and pain, leading to the elevation of blood pressure (BP) and heart rate (HR). Such effects may be exaggerated and cause life-threatening accidents in patients with hypertension. Therefore, the pain and anxiety management of these patients is imperative. Virtual reality (VR) has been demonstrated to be a distraction method to relieve anxiety and pain in clinical operations. Thus, we hypothesized that VR can control the elevation of BP and HR in patients with hypertension. In this study, 96 eligible patients with controlled hypertension who needed tooth extraction were randomized to the VR or standard care group by stratified randomization of anxiety grade and gender. Their BP and HR were dynamically monitored. The corresponding systolic and diastolic BP and HR values were selected when systolic BP was at the highest point of the process. BP was converted into mean arterial pressure (MAP) for comparison per the following formula: MAP = (systolic BP + 2 × diastolic BP)/3. Statistical analyses were by intention to treat and conducted in SPSS. Nonparametric rank sum tests were used to compare the difference of ΔMAP and ΔHR between the VR and standard care groups. Multivariate linear regression was applied to evaluate the effect of VR on ΔMAP and ΔHR. The results showed that the VR technique significantly decreased the elevation of MAP (P < 0.001) and HR (P < 0.001), and this effect was found even after adjusting for baseline characteristics and additional surgical procedures (ΔMAP, P < 0.001, R2 = 0.276; ΔHR, P < 0.001, R2 = 0.152). VR did not increase the incidence of adverse events (P = 0.677). In conclusion, the VR technique was effective in controlling BP and HR within an acceptable range and can help manage BP and HR during tooth extraction for patients with hypertension (Chinese Clinical Trial Registry: ChiCTR2100042132).
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Affiliation(s)
- Z Qin
- Department of Oral and Maxillofacial Surgery, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
- Department of General Dentistry, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
| | - C Zhou
- Department of Emergency, The Eighth Affiliated Hospital, Sun Yat-sen University, Shenzhen, China
| | - Y Zhu
- Clinical Research Center, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
| | - Y Wang
- Department of Oral and Maxillofacial Surgery, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
- Department of General Dentistry, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
| | - H Cao
- Department of Oral and Maxillofacial Surgery, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
- Department of General Dentistry, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
| | - W Li
- Department of Critical Medicine, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
| | - Z Huang
- Department of Oral and Maxillofacial Surgery, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
- Department of General Dentistry, Sun Yat-sen Memorial Hospital, Sun Yat-sen University, Guangzhou, China
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Lu Y, Huang J, Zhang Y, Huang Z, Yan W, Zhou T, Wang Z, Liao L, Cao H, Tan B. Therapeutic Effects of Berberine Hydrochloride on Stress-Induced Diarrhea-Predominant Irritable Bowel Syndrome Rats by Inhibiting Neurotransmission in Colonic Smooth Muscle. Front Pharmacol 2021; 12:596686. [PMID: 34594213 PMCID: PMC8476869 DOI: 10.3389/fphar.2021.596686] [Citation(s) in RCA: 9] [Impact Index Per Article: 3.0] [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: 08/20/2020] [Accepted: 09/01/2021] [Indexed: 11/13/2022] Open
Abstract
The etiology of diarrhea-predominant irritable bowel syndrome (IBS-D) is complicated and closely related to neurotransmission in the gastrointestinal (GI) tract. Developing new strategies for treating this disease is a major challenge for IBS-D research. Berberine hydrochloride (BBH), the derivative of berberine, is a herbal constituent used to treat IBS. Previous studies have shown that BBH has potential anti-inflammatory, antibacterial, analgesic, and antidiarrheal effects and a wide range of biological activities, especially in regulating the release of some neurotransmitters. A modified IBS-D rat model induced by chronic restraint stress was used in all experiments to study the effects of BBH on the GI tract. This study measured the abdominal withdrawal reflex (AWR) response to graded colorectal distention (CRD; 20, 40, 60, and 80 mmHg) and observed the fecal areas of stress-induced IBS-D model. Experiments were conducted using organ bath techniques, which were performed in vitro using strips of colonic longitudinal smooth muscle. Inhibitory and excitatory neurotransmitter agents were added to each organ bath to observe contractile responses on the strips and the treatment effect exerted by BBH. The IBS-D rat model was successfully induced by chronic restraint stress, which resulted in an increased defecation frequency and visceral hypersensitivity similar to that of humans. BBH could reduce 4-h fecal areas and AWR response to CRD in IBS-D. The stress-induced IBS-D model showed upregulated colonic mRNA expression levels of 5-hydroxytryptamine-3A receptor and downregulated expression levels of neuronal nitric oxide synthase. Meanwhile, BBH could reverse this outcome. The responses of substances that regulate the contraction induced by related neurotransmission in the longitudinal smooth muscle of IBS-D colon (including the agonist of acetylcholine, carbachol; NOS inhibitor, L-NAME; and P2Y1 receptor antagonist, MRS2500) can be inhibited by BBH. In summary, BBH promotes defecation frequency and visceral hypersensitivity in IBS-D and exerts inhibitory effects on contractile responses in colonic longitudinal smooth muscle. Thus, BBH may represent a new therapeutic approach for treating IBS-D.
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Affiliation(s)
- Yulin Lu
- Research Center for Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Jingjing Huang
- Research Center for Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Yao Zhang
- School of Chinese Materia Medica, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Zitong Huang
- Research Center for Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Weiming Yan
- The Third Clinical Medical College, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Tianran Zhou
- The Fourth Clinical Medical College, Guangzhou University of Chinese Medicine, Shenzhen, China
| | - Zhesheng Wang
- Research Center for Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Lu Liao
- Research Center for Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Hongying Cao
- School of Chinese Materia Medica, Guangzhou University of Chinese Medicine, Guangzhou, China
| | - Bo Tan
- Research Center for Integrative Medicine, School of Basic Medical Sciences, Guangzhou University of Chinese Medicine, Guangzhou, China
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Gu JY, Shi HT, Yang LX, Shen YQ, Wang ZX, Feng Q, Wang M, Cao H. [Clinical significance of the deep learning algorithm based on contrast-enhanced CT in the differential diagnosis of gastric gastrointestinal stromal tumors with a diameter ≤ 5 cm]. Zhonghua Wei Chang Wai Ke Za Zhi 2021; 24:796-803. [PMID: 34530561 DOI: 10.3760/cma.j.cn.441530-20210706-00267] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 11/05/2022]
Abstract
Objective: Contrast-enhanced CT is an important method of preoperative diagnosis and evaluation for the malignant potential of gastric submucosal tumor (SMT). It has a high diagnostic accuracy rate in differentiating gastric gastrointestinal stromal tumor (GIST) with a diameter greater than 5 cm from gastric benign SMT. This study aimed to use deep learning algorithms to establish a diagnosis model (GISTNet) based on contrast-enhanced CT and evaluate its diagnostic value in distinguishing gastric GIST with a diameter ≤ 5 cm and other gastric SMT before surgery. Methods: A diagnostic test study was carried out. Clinicopathological data of 181 patients undergoing resection with postoperative pathological diagnosis of gastric SMT with a diameter ≤ 5 cm at Department of Gastrointestinal Surgery of Renji Hospital from September 2016 to April 2021 were retrospectively collected. After excluding 13 patients without preoperative CT or with poor CT imaging quality, a total of 168 patients were enrolled in this study, of whom, 107 were GIST while 61 were benign SMT (non-GIST), including 27 leiomyomas, 24 schwannomas, 6 heterotopic pancreas and 4 lipomas. Inclusion criteria were as follows: (1) gastric SMT was diagnosed by contrast-enhanced CT before surgery; (2) preoperative gastroscopic examination and biopsy showed no abnormal cells; (3) complete clinical and pathological data. Exclusion criteria were as follows: (1) patients received anti-tumor therapy before surgery; (2) without preoperative CT or with poor CT imaging quality due to any reason; (3) except GIST, other gastric malignant tumors were pathologically diagnosed after surgery. Based on the hold-out method, 148 patients were randomly selected as the training set and 20 patients as the test set of the GISTNet diagnosis model. After the GISTNet model was established, 5 indicators were used for evaluation in the test set, including sensitivity, specificity, positive predictive value, negative predictive value and the area under the receiver operating curve (AUC). Then GISTNet diagnosis model was compared with the GIST-risk scoring model based on traditional CT features. Besides, in order to compare the accuracy of the GISTNet diagnosis model and the imaging doctors in the diagnosis of gastric SMT imaging, 3 radiologists with 3, 9 and 19 years of work experience, respectively, blinded to clinical and pathological information, tested and judged the samples. The accuracy rate between the three doctors and the GISTNet model was compared. Results: The GISTNet model yielded an AUC of 0.900 (95% CI: 0.827-0.973) in the test set. When the threshold value was 0.345, the sensitivity specificity, positive and negative predictive values of the GISTNet diagnosis model was 100%, 67%, 75% and 100%, respectively. The accuracy rate of the GISTNet diagnosis model was better than that of the GIST-risk model and the manual readings from two radiologists with 3 years and 9 years of work experience (83% vs. 75%, 60%, 65%), and was close to the manual reading of the radiologist with 19 years of work experience (83% vs. 80%). Conclusion: The deep learning algorithm based on contrast-enhanced CT has favorable and reliable diagnostic accuracy in distinguishing gastric GIST with a diameter ≤ 5 cm and other gastric SMT before operation.
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Affiliation(s)
- J Y Gu
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - H T Shi
- Shanghai Jiaotong University School of Medicine, Shanghai 200025, China
| | - L X Yang
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - Y Q Shen
- School of Mathematical Sciences, Zhiyuan Innovative Research Center, Shanghai Jiaotong University, Shanghai 200240, China
| | - Z X Wang
- Shanghai Jiaotong University School of Medicine, Shanghai 200025, China
| | - Q Feng
- Department of Radiology, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - M Wang
- 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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49
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Cao H, Wang M. [Act following etiquette and change with time: analysis and discussion on the difference between the current guidelines and clinical practice of gastrointestinal stromal tumor]. Zhonghua Wei Chang Wai Ke Za Zhi 2021; 24:749-757. [PMID: 34530554 DOI: 10.3760/cma.j.cn.441530-20210618-00350] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 11/05/2022]
Abstract
Gastrointestinal stromal tumor (GIST) is the most common mesenchymal tumor in the gastrointestinal tract. At present, many professional academic groups and associations at home and abroad have released guidelines for the diagnosis and treatment of GIST. In 2020, Gastrointestinal Stromal Tumor Expert Committee of China Society of Clinical Oncology (CSCO) issued the first "CSCO gastrointestinal stromal tumor diagnosis and treatment guidelines" in China. In the same year, NCCN also released the first "NCCN guideline for the diagnosis and treatment of gastrointestinal stromal tumors (first edition in 2021)" by separating GIST-related content from the guideline for soft tissue sarcoma. However, there are many inconsistencies between the guidelines' recommendation and clinical practice in China. For example, in the aspect of diagnosis, the emphasis on and implementation of molecular detection are variable, the format of molecular detection report is not unified or standardized, the selection of detection methods is inappropriate, the diagnosis of wild-type GIST is not standardized, the risk assessment is improper, and the use of EUS-FNA is relatively seldom; in the aspect of drug therapy, there are some problems, such as the lack of standardization in dose and course of targeted drugs, and off-label medication such as cross line therapy; in terms of surgical treatment, there are also some problems, such as the clinical application scenarios of laparoscopic surgery exceed the recommendations of the guidelines, and the general description of surgical intervention of advanced GIST in the guidelines cannot well guide specific clinical practice. In this context, on the one hand, clinicians need to understand the academic frontier and standardize their medical behavior with the latest guidelines; on the other hand, clinicians need to consider the scientific rationale and accessibility of treatment on some clinical problems that are not clear in the guidelines, and take whether patients can benefit the most as the criteria.
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Affiliation(s)
- H Cao
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - M Wang
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
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50
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Ni B, Yang LX, Wang M, Cao H. [Identification and inner relation between gastrointestinal stromal tumor and intra-abdominal desmoid tumor]. Zhonghua Wei Chang Wai Ke Za Zhi 2021; 24:830-835. [PMID: 34530567 DOI: 10.3760/cma.j.cn.441530-20210704-00260] [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: 11/05/2022]
Abstract
Intra-abdominal desmoid tumor (IADT) and gastrointestinal stromal tumor (GIST) are both mesenchymal tumors mostly found in gastrointestinal tracts and easily misdiagnosed, which would directly damage the survival prognosis and quality of life of patients. With the advent of the era of precision medicine, the understanding of the above two diseases is more in-depth, and the requirements for accurate diagnosis and individualized precision treatment are more stringent. Moreover, there seems to be some internal relationship between IADT and GIST, and the lack of systematic research and discussion makes clinical decision-making and patient management easy to fall into traps and misunderstandings. Therefore, this paper reviews the clinical characteristics, pathogenesis and treatments of the two, and explore their differences and internal relations, so as to provide research and practical reference for promoting more precise and individualized diagnosis and treatment regimens.
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Affiliation(s)
- B Ni
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - L X Yang
- Department of Gastrointestinal Surgery, Renji Hospital, Shanghai Jiaotong University School of Medicine, Shanghai 200127, China
| | - M Wang
- 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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