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Kriechbaum SD, Birmes J, Wiedenroth CB, Gruen D, Vietheer J, Richter MJ, Guth S, Roller F, Liebetrau C, Hamm CW, Keller T, Rieth A. Exercise MR-proANP unmasks latent right heart failure in CTEPH. Eur Heart J 2022. [DOI: 10.1093/eurheartj/ehac544.915] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
Abstract
Abstract
Background
Chronic right heart failure is the major determinant of outcome in chronic thromboembolic pulmonary hypertension (CTEPH). Thus, its early detection is crucial for optimal patient management. Hemodynamic assessment with invasive right heart catheterization and the measurement of natriuretic peptides at rest are established diagnostic tools in this context. An elevated right atrial pressure (RAP) is a sensitive parameter of right right heart failure. Mid-regional pro-atrial natriuretic peptide (MR-proANP) is a natriuretic peptide that reflects right atrial stress levels.
There is a growing recognition of exercise diagnostics in the assessment of right heart failure, particularly in patients with normal or borderline findings at rest. There are no data on the dynamics of MR-proANP in correlation to RAP during physical exercise.
Purpose
The present study was designed to investigate the dynamics of RAP and MR-proANP during physical exercise in patients with CTEPH and to determine whether these parameters might serve as a tool to measure exercise-dependent atrial stress as an indicator of right heart failure.
Methods
This observational cohort study included 100 CTEPH patients who underwent right heart catheterization during physical exercise (eRHC). Blood samples for MR-proANP measurement were taken prior, during, and after eRHC. MR-proANP levels were correlated to RAP levels at rest, at peak exercise (eRAP), and during recovery. RAP at rest ≤7 mmHg was defined as normal and eRAP >15 mmHg as suggestive of right heart failure.
Results
During eRHC mean RAP increased from 6±4 mmHg to 16±7 mmHg (p<0.001). MR-proANP levels and dynamics correlated with RAP at rest (rs=0.61; p<0.001; figure 1a) and at peak exercise (rs=0.66; p<0.001; Figure 1b). Furthermore, the relative percent increase in MR-proANP correlated with the relative percent increase in eRAP (rs=0.52; p<0.001; Figure 1c) Logistic regression analysis revealed the peak MR-proANP level (B=0.058; p=0.004) and the right atrial area (B=0.389; p<0.001) to be associated with eRAP dynamics. A peak MR-proANP level ≥139 pmol/L (AUC=0.81) and recovery level ≥159 pmol/L (AUC=0.82) predicted an eRAP >15 mmHg. Physical exercise unmasked RH failure in 39% of patients with normal RAP at rest; they were also characterized by a more distinct increase in MR-proANP levels (p=0.005) and higher peak (p<0.001) and recovery levels (p<0.001).
Conclusions
RAP and MR-proANP dynamics unmask manifest and latent right heart failure in CTEPH patients, which may be useful in estimating prognosis.
Funding Acknowledgement
Type of funding sources: Foundation. Main funding source(s): SFB 1213 area CP-01 projectWilliam G. Kerckhoff-FoundationKerckhoff Heart Research Institute (KHFI)German Center for Cardiovascular Research (DZHK)
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Affiliation(s)
- S D Kriechbaum
- Kerckhoff Heart and Thorax Center, Department of Cardiology , Bad Nauheim , Germany
| | - J Birmes
- Kerckhoff Heart and Thorax Center, Department of Cardiology , Bad Nauheim , Germany
| | - C B Wiedenroth
- Kerckhoff Heart and Thorax Center, Department of Thoracic Surgery , Bad Nauheim , Germany
| | - D Gruen
- University Hospital Giessen and Marburg, Medical Clinic I, Cardiology , Giessen , Germany
| | - J Vietheer
- Kerckhoff Heart and Thorax Center, Department of Cardiology , Bad Nauheim , Germany
| | - M J Richter
- University Hospital Giessen and Marburg, Medical Clinic II, Pneumology , Giessen , Germany
| | - S Guth
- Kerckhoff Heart and Thorax Center, Department of Thoracic Surgery , Bad Nauheim , Germany
| | - F Roller
- University Hospital Giessen and Marburg, Radiology , Giessen , Germany
| | - C Liebetrau
- CCB am Markus Hospital, Cardiology , Frankfurt am Main , Germany
| | - C W Hamm
- Kerckhoff Heart and Thorax Center, Department of Cardiology , Bad Nauheim , Germany
| | - T Keller
- University Hospital Giessen and Marburg, Medical Clinic I, Cardiology , Giessen , Germany
| | - A Rieth
- Kerckhoff Heart and Thorax Center, Department of Cardiology , Bad Nauheim , Germany
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Pandey S, Krause E, DeRose J, MacCrann N, Jain B, Crocce M, Blazek J, Choi A, Huang H, To C, Fang X, Elvin-Poole J, Prat J, Porredon A, Secco L, Rodriguez-Monroy M, Weaverdyck N, Park Y, Raveri M, Rozo E, Rykoff E, Bernstein G, Sánchez C, Jarvis M, Troxel M, Zacharegkas G, Chang C, Alarcon A, Alves O, Amon A, Andrade-Oliveira F, Baxter E, Bechtol K, Becker M, Camacho H, Campos A, Carnero Rosell A, Carrasco Kind M, Cawthon R, Chen R, Chintalapati P, Davis C, Di Valentino E, Diehl H, Dodelson S, Doux C, Drlica-Wagner A, Eckert K, Eifler T, Elsner F, Everett S, Farahi A, Ferté A, Fosalba P, Friedrich O, Gatti M, Giannini G, Gruen D, Gruendl R, Harrison I, Hartley W, Huff E, Huterer D, Kovacs A, Leget P, McCullough J, Muir J, Myles J, Navarro-Alsina A, Omori Y, Rollins R, Roodman A, Rosenfeld R, Sevilla-Noarbe I, Sheldon E, Shin T, Troja A, Tutusaus I, Varga T, Wechsler R, Yanny B, Yin B, Zhang Y, Zuntz J, Abbott T, Aguena M, Allam S, Annis J, Bacon D, Bertin E, Brooks D, Burke D, Carretero J, Conselice C, Costanzi M, da Costa L, Pereira M, De Vicente J, Dietrich J, Doel P, Evrard A, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, James D, Jeltema T, Kuehn K, Kuropatkin N, Lahav O, Lima M, Lin H, Maia M, Marshall J, Melchior P, Menanteau F, Miller C, Miquel R, Mohr J, Morgan R, Palmese A, Paz-Chinchón F, Petravick D, Pieres A, Plazas Malagón A, Sanchez E, Scarpine V, Serrano S, Smith M, Soares-Santos M, Suchyta E, Tarle G, Thomas D, Weller J. Dark Energy Survey year 3 results: Constraints on cosmological parameters and galaxy-bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.043520] [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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Holtkamp F, Gruen D, Frey A, Jahns V, Jahns R, Gassenmaier T, Hamm C, Frantz S, Keller T, Klingenberg R. Does a 6-month change in circulating biomarkers improve the prognostic power of baseline values for predicting cardiac MRI pathologies in patients with STEMI? Atherosclerosis 2022. [DOI: 10.1016/j.atherosclerosis.2022.06.221] [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] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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Abbott T, Aguena M, Alarcon A, Allam S, Alves O, Amon A, Andrade-Oliveira F, Annis J, Avila S, Bacon D, Baxter E, Bechtol K, Becker M, Bernstein G, Bhargava S, Birrer S, Blazek J, Brandao-Souza A, Bridle S, Brooks D, Buckley-Geer E, Burke D, Camacho H, Campos A, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Cawthon R, Chang C, Chen A, Chen R, Choi A, Conselice C, Cordero J, Costanzi M, Crocce M, da Costa L, da Silva Pereira M, Davis C, Davis T, De Vicente J, DeRose J, Desai S, Di Valentino E, Diehl H, Dietrich J, Dodelson S, Doel P, Doux C, Drlica-Wagner A, Eckert K, Eifler T, Elsner F, Elvin-Poole J, Everett S, Evrard A, Fang X, Farahi A, Fernandez E, Ferrero I, Ferté A, Fosalba P, Friedrich O, Frieman J, García-Bellido J, Gatti M, Gaztanaga E, Gerdes D, Giannantonio T, Giannini G, Gruen D, Gruendl R, Gschwend J, Gutierrez G, Harrison I, Hartley W, Herner K, Hinton S, Hollowood D, Honscheid K, Hoyle B, Huff E, Huterer D, Jain B, James D, Jarvis M, Jeffrey N, Jeltema T, Kovacs A, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Leget PF, Lemos P, Liddle A, Lidman C, Lima M, Lin H, MacCrann N, Maia M, Marshall J, Martini P, McCullough J, Melchior P, Mena-Fernández J, Menanteau F, Miquel R, Mohr J, Morgan R, Muir J, Myles J, Nadathur S, Navarro-Alsina A, Nichol R, Ogando R, Omori Y, Palmese A, Pandey S, Park Y, Paz-Chinchón F, Petravick D, Pieres A, Plazas Malagón A, Porredon A, Prat J, Raveri M, Rodriguez-Monroy M, Rollins R, Romer A, Roodman A, Rosenfeld R, Ross A, Rykoff E, Samuroff S, Sánchez C, Sanchez E, Sanchez J, Sanchez Cid D, Scarpine V, Schubnell M, Scolnic D, Secco L, Serrano S, Sevilla-Noarbe I, Sheldon E, Shin T, Smith M, Soares-Santos M, Suchyta E, Swanson M, Tabbutt M, Tarle G, Thomas D, To C, Troja A, Troxel M, Tucker D, Tutusaus I, Varga T, Walker A, Weaverdyck N, Wechsler R, Weller J, Yanny B, Yin B, Zhang Y, Zuntz J. Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.023520] [Citation(s) in RCA: 106] [Impact Index Per Article: 53.0] [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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Amon A, Gruen D, Troxel M, MacCrann N, Dodelson S, Choi A, Doux C, Secco L, Samuroff S, Krause E, Cordero J, Myles J, DeRose J, Wechsler R, Gatti M, Navarro-Alsina A, Bernstein G, Jain B, Blazek J, Alarcon A, Ferté A, Lemos P, Raveri M, Campos A, Prat J, Sánchez C, Jarvis M, Alves O, Andrade-Oliveira F, Baxter E, Bechtol K, Becker M, Bridle S, Camacho H, Carnero Rosell A, Carrasco Kind M, Cawthon R, Chang C, Chen R, Chintalapati P, Crocce M, Davis C, Diehl H, Drlica-Wagner A, Eckert K, Eifler T, Elvin-Poole J, Everett S, Fang X, Fosalba P, Friedrich O, Gaztanaga E, Giannini G, Gruendl R, Harrison I, Hartley W, Herner K, Huang H, Huff E, Huterer D, Kuropatkin N, Leget P, Liddle A, McCullough J, Muir J, Pandey S, Park Y, Porredon A, Refregier A, Rollins R, Roodman A, Rosenfeld R, Ross A, Rykoff E, Sanchez J, Sevilla-Noarbe I, Sheldon E, Shin T, Troja A, Tutusaus I, Tutusaus I, Varga T, Weaverdyck N, Yanny B, Yin B, Zhang Y, Zuntz J, Aguena M, Allam S, Annis J, Bacon D, Bertin E, Bhargava S, Brooks D, Buckley-Geer E, Burke D, Carretero J, Costanzi M, da Costa L, Pereira M, De Vicente J, Desai S, Dietrich J, Doel P, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, Hoyle B, James D, Kron R, Kuehn K, Lahav O, Lima M, Lin H, Maia M, Marshall J, Martini P, Melchior P, Menanteau F, Miquel R, Mohr J, Morgan R, Ogando R, Palmese A, Paz-Chinchón F, Petravick D, Pieres A, Romer A, Sanchez E, Scarpine V, Schubnell M, Serrano S, Smith M, Soares-Santos M, Tarle G, Thomas D, To C, Weller J. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.023514] [Citation(s) in RCA: 42] [Impact Index Per Article: 21.0] [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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Prim J, Uhlemann T, Gumpfer N, Gruen D, Wegener S, Krug S, Hannig J, Keller T, Guckert M. A data-pipeline processing electrocardiogram recordings for use in artificial intelligence algorithms. Eur Heart J 2021. [DOI: 10.1093/eurheartj/ehab724.3041] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
Abstract
Abstract
Introduction
Artificial intelligence (AI) can be used for various tasks in medicine and specifically in cardiology. Medical data such as electrocardiogram recordings (ECGs) are widely used and universally accepted as diagnostic and prognostic tools. It has been shown that deep learning methods using ECGs yield excellent results detecting cardiac pathologies. A significant amount of reliable data is required for supervised learning algorithms such as deep learning models. However, only a small fraction of ECG data generated in daily practice is available in a fully digital and machine-readable format, such as XML. Frequently, used ECG devices produce PDF files or even paper-based print outs, which need to be digitised later for inclusion in clinical information systems. Such ECGs cannot be used without further effort for training or application of deep learning models. Therefore, aim of the present project was to develop a data-pipeline that generates machine-readable ECG data for AI use data irrespective of the initial ECG format.
Methods
We propose an end-to-end pipeline that can not only process data from modern digital ECG devices but is also capable of extracting all necessary information from PDF files (both scanned hard copies and digitally generated PDFs) (see Figure 1). By using different techniques including adaption of open source libraries for vectorisation of image data, and modern computer vision technologies, such as optical character recognition (OCR), our pipeline is able to flexibly process data from different recording devices and read both data in PDF format and data from native digital devices delivered in XML. The processed files from various sources are either saved as a common and easily accessible CSV file format, or are processed directly with deep learning models (see Figure 2).
Results
The developed data-pipeline was validated using data from a set of 113 12-lead ECGs for which data was available in multiple formats. Each format dataset was separately processed by our pipeline and then used for training and validation of a deep learning architecture for myocardial scar detection based on raw ECG signals. The quality of the extraction process by our pipeline was assessed by the respective deep learning models with their prediction capability depicted by receiver operator characteristic analyses (ROC). Comparing the benchmark model that was generated from XML data against a model that was purely trained on PDF data processed by the pipeline shows that both models produced comparable results, reaching area under the curve (AUC) values of 0:79±0:10 (XML) and 0:83±0:07 (PDF).
Conclusion
The data pipeline facilitates acceleration of ECG-based AI research and application of AI algorithms by providing access to ECG data irrespective of the format of the stored ECG. Future work will focus on independent validation as well as expanding this pipeline to include additional ECG types.
Funding Acknowledgement
Type of funding sources: Public Institution(s). Main funding source(s): Flexi Funds by Forschungscampus Mittelhessen
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Affiliation(s)
- J Prim
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum für Informationstechnologie, Giessen, Germany
| | - T Uhlemann
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum für Informationstechnologie, Giessen, Germany
| | - N Gumpfer
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum für Informationstechnologie, Giessen, Germany
| | - D Gruen
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Giessen, Germany
| | - S Wegener
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Giessen, Germany
| | - S Krug
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum für Informationstechnologie, Giessen, Germany
| | - J Hannig
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum für Informationstechnologie, Giessen, Germany
| | - T Keller
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Giessen, Germany
| | - M Guckert
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum für Informationstechnologie, Giessen, Germany
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Gumpfer N, Wegener S, Prim J, Gruen D, Hannig J, Keller T, Guckert M. On the importance of representative datasets in ECG-based artificial intelligence. Eur Heart J 2021. [DOI: 10.1093/eurheartj/ehab724.3060] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
Abstract
Abstract
Background/Introduction
ECG-based artificial intelligence (AI) is an emerging field in digital cardiology. Training on diseased records vs. healthy controls is common practice. We aimed to evaluate if such an approach can lead to unwanted behaviour in real-world settings and thus unnecessarily reduce diagnostic precision of the developed AI model.
Purpose
Several studies have shown that deep neural networks are able to exceed performance of medical experts. However, when these models are applied to different cohorts, results vary strongly. We hypothesise that this is because the datasets used for training were not representative for the target population.
Methods
Based on the public ECG database PTB-XL we sampled three distinct subsets of n=150 records representing ECG groups labelled for diagnoses 'old myocardial infarction' (M), 'normal ECG' (N), or 'other cardiac abnormality' (O). These groups were combined to three datasets ([M, N] (n=300), [M, O] (n=300), [M, N, O] (n=450)), representing different approaches to data sampling. On each dataset, we trained a separate but equally structured deep neural network using 100-fold bootstrapping. The diagnostic performance of each model was validated on unseen data from all datasets with sensitivity, specificity and area under the receiver operator characteristic curve.
Results
Evaluation of the three differently trained models shows best diagnostic performance on the M vs. N records and worst on the M vs. O records. However, in the out-of-dataset setting, the best-performing model (trained on [M, N]) shows weaker performance on the [M, N, O] and [M, O] datasets. Sensitivity for the same model remained equal, as identical M records were used throughout corresponding bootstrapping folds. Detailed results are presented in Table 1.
Conclusions
Our results suggest that the model trained on a dataset including only diseased records vs. healthy controls [M, N] learned to recognise healthy (N) instead of diseased (M) records, which explains why it performed poorly on datasets including records showing other cardiac abnormalities (O). Such behaviour is a common problem in AI and requires special attention in dataset sampling. For small cohorts, it is tempting to increase the amount of training data by using healthy controls. However, we have shown that this can be a poor option, since classifiers can more easily rely on features that are not actually related to the target disease. Training and validation of classifiers should therefore be performed on representative datasets that are as close as possible to the target population.
Funding Acknowledgement
Type of funding sources: Public Institution(s). Main funding source(s): Forschungscampus Mittelhessen, Flexi Funds Table 1
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Affiliation(s)
- N Gumpfer
- University of Applied Sciences Mittelhessen, Kompetenzzentrum für Informationstechnologie, Workgroup Cognitive Information Systems, Giessen, Germany
| | - S Wegener
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - J Prim
- University of Applied Sciences Mittelhessen, Kompetenzzentrum für Informationstechnologie, Workgroup Cognitive Information Systems, Giessen, Germany
| | - D Gruen
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - J Hannig
- University of Applied Sciences Mittelhessen, Kompetenzzentrum für Informationstechnologie, Workgroup Cognitive Information Systems, Giessen, Germany
| | - T Keller
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - M Guckert
- University of Applied Sciences Mittelhessen, Kompetenzzentrum für Informationstechnologie, Workgroup Cognitive Information Systems, Giessen, Germany
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Wegener S, Gruen D, Prim J, Gumpfer N, Wolter JS, Hamm CW, Liebetrau C, Hannig J, Guckert M, Keller T. Predicting mortality in cardiovascular patients using electrocardiogram data and artificial intelligence. Eur Heart J 2021. [DOI: 10.1093/eurheartj/ehab724.1132] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Abstract
Background/Introduction
The electrocardiogram (ECG) is an ubiquitously used non-invasive tool for diagnosis and risk prediction in cardiology, granting deep extensive insights into the heart. Artificial intelligence (AI) is a modern resource allowing the processing of vast complex datasets in a way that is comparable to humans. Risk stratification in cardiovascular patients is mainly based on scoring systems, such as the ESC-SCORE, relying on traditional risk variables like cholesterol levels or arterial hypertension, rather than actual cardiac structure and function. Goal of this project was to predict mortality using AI in patients with cardiovascular risk based on the current cardiac situation represented by a standard 12-lead ECG recording.
Methods
The study population is based on an ongoing registry that started in 2010 and enrolled patients scheduled for an invasive coronary angiography due to suspected chronic coronary syndrome. Data of the following study patients were analysed: enrolment within the first two study years with available long-term follow-up data on the outcome measure overall mortality, availability of an ECG at admission without pacemaker stimulation and availability of all variables needed to calculate the ESC-SCORE (in the version weighed for a German population) as comparison. This led to a cohort of 720 patients, of whom 70 died within the follow-up period. Information on presence of a relevant coronary artery disease (CAD) was available for all patients, to differentiate between primary and secondary prevention. A deep learning architecture that was previously developed to detect myocardial scar in raw ECG time-series data was used. This model was trained with 1400 ECG recordings, from the publicly available PTB-XL dataset with 700 of those ECGs labelled for acute, recent or old myocardial infarction while 700 were labelled as healthy. This pre-trained model was then applied to our study cohort to predict long-term mortality based on a single 12-lead ECG obtained at admission.
Results
For mortality prediction in patients without CAD (primary prevention) the AI model compares to the ESC-SCORE with an AUROC of 0.606 vs 0.584. For CAD patients (secondary prevention) the AI model compares with an AUROC of 0.612 vs 0.658. Detailed results are presented in Table 1.
Conclusion(s)
Our data underlines the potential of an AI based approach, predicting mortality in cardiovascular patients using only single 12-lead ECG recordings. Additionally, our model achieved similar predictive information to established risk classification systems, such as the ESC-SCORE. Since data acquisition is still ongoing, we will continue to improve our model. In future work training AI to specifically predict mortality while also exploring explainable AI could lead to breakthrough findings in ECG interpretation.
Funding Acknowledgement
Type of funding sources: Public Institution(s). Main funding source(s): FlexiFunds by Forschungscampus Mittelhessen
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Affiliation(s)
- S Wegener
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - D Gruen
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - J Prim
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - N Gumpfer
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - J S Wolter
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - C W Hamm
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - C Liebetrau
- CardioVascular Center Bethanien (CCB), Department of Cardiology, Frankfurt, Germany
| | - J Hannig
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - M Guckert
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - T Keller
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
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Wegener S, Schmidt T, Prim J, Gumpfer N, Gruen D, Hannig J, Guckert M, Keller T. Detecting a broader spectrum of cardiac pathologies in electrocardiogram data by applying a deep neural network designed to detect a specific cardiac disease. Eur Heart J 2021. [DOI: 10.1093/eurheartj/ehab724.3063] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
Abstract
Background/Introduction
The electrocardiogram (ECG) is a widely used and inexpensive tool that provides extensive insights into the cardiac structure and function. Artificial intelligence (AI) algorithms, especially deep learning (DL) models, are efficient computer based instruments with which large and complex datasets can be processed for identification of e.g. specific diseases. PhysioNet is a NIH research resource for complex signals including a large amount of labelled ECG time-series data. Our aim was to evaluate the diagnostic performance of an AI architecture developed to detect a specific cardiac pathology in a large ECG data set including a broad range of cardiac abnormalities.
Methods
The PhysioNet ECG dataset provided as part of the PhysioNet Challenge 2020 consists of five distinct databases with a total of 43100 12-Lead ECG recordings of varying length stemming from patients from China, Russia, Europe and the United States. Each ECG recording is annotated with diagnoses based on a set of 111 possible labels, which express either a cardiac pathology, e.g. atrial flutter or anterior wall ischemia, or unspecific changes in the ECG, e.g. a prolonged qt interval or low qrs voltages. Based on these labels we defined 10 groups merging PhysioNet labels describing related cardiac abnormalities (see Table 1). We adapted a recently published DL model which used raw ECG time-series data of all 12-leads rather than extracted features as model input. This DL model was adapted to the larger number of output variables and then trained on 80% (n=34480 ECGs) of the PhysioNet dataset. The remaining 20% (n=8620 ECGs) of the PhysioNet dataset were used to evaluate the diagnostic performance of the AI model. Sensitivities, specificities and the areas under the receiver operator characteristic curves (AUROC) were used as performance metrices.
Results
The AI model, that was initially designed to detect a specific cardiac pathology, performed well in the large PhysioNet dataset providing AUROCs ranging from 0.78 to 0.95 to detect the defined 10 cardiac abnormality groups. Interestingly, the AI model was able to detect disease groups with changes in the chronological sequence of the ECG, e.g. arrhythmia, with comparable precision as disease groups associated primarily with changes in the ECG amplitude like e.g. ischemia. Detailed results are presented in Table 2.
Conclusion(s)
Our evaluation shows that an AI model that uses raw ECG time-series data rather than extracted features as model input can be easily transferred to other large datasets with different prediction variables. This might also serve as a proof of concept that raw data instead of pre-selected features should be used as model input if developing AI applications for medical use cases.
Funding Acknowledgement
Type of funding sources: Public Institution(s). Main funding source(s): FlexiFunds by Forschungscampus Mittelhessen
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Affiliation(s)
- S Wegener
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - T Schmidt
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - J Prim
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - N Gumpfer
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - D Gruen
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
| | - J Hannig
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - M Guckert
- University of Applied Sciences Mittelhessen, Cognitive Information Systems, Kompetenzzentrum fuer Informationstechnologie, Giessen, Germany
| | - T Keller
- Justus-Liebig University of Giessen, Department of Internal Medicine I, Cardiology, Giessen, Germany
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Saiz FS, Brotman D, Preininger A, Felix W, Huang H, Gruen D, Jackson G. OA19.04 Potential Clinical and Economic Impact of Missed Lung Nodules – A Claims Database Analysis. J Thorac Oncol 2021. [DOI: 10.1016/j.jtho.2021.08.100] [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: 11/30/2022]
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To C, Krause E, Rozo E, Wu H, Gruen D, Wechsler RH, Eifler TF, Rykoff ES, Costanzi M, Becker MR, Bernstein GM, Blazek J, Bocquet S, Bridle SL, Cawthon R, Choi A, Crocce M, Davis C, DeRose J, Drlica-Wagner A, Elvin-Poole J, Fang X, Farahi A, Friedrich O, Gatti M, Gaztanaga E, Giannantonio T, Hartley WG, Hoyle B, Jarvis M, MacCrann N, McClintock T, Miranda V, Pereira MES, Park Y, Porredon A, Prat J, Rau MM, Ross AJ, Samuroff S, Sánchez C, Sevilla-Noarbe I, Sheldon E, Troxel MA, Varga TN, Vielzeuf P, Zhang Y, Zuntz J, Abbott TMC, Aguena M, Amon A, Annis J, Avila S, Bertin E, Bhargava S, Brooks D, Burke DL, Carnero Rosell A, Carrasco Kind M, Carretero J, Chang C, Conselice C, da Costa LN, Davis TM, Desai S, Diehl HT, Dietrich JP, Everett S, Evrard AE, Ferrero I, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gruendl RA, Gutierrez G, Hinton SR, Hollowood DL, Honscheid K, Huterer D, James DJ, Jeltema T, Kron R, Kuehn K, Kuropatkin N, Lima M, Maia MAG, Marshall JL, Menanteau F, Miquel R, Morgan R, Muir J, Myles J, Palmese A, Paz-Chinchón F, Plazas AA, Romer AK, Roodman A, Sanchez E, Santiago B, Scarpine V, Serrano S, Smith M, Suchyta E, Swanson MEC, Tarle G, Thomas D, Tucker DL, Weller J, Wester W, Wilkinson RD. Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations. Phys Rev Lett 2021; 126:141301. [PMID: 33891448 DOI: 10.1103/physrevlett.126.141301] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/06/2020] [Revised: 01/07/2021] [Accepted: 02/23/2021] [Indexed: 06/12/2023]
Abstract
We present the first joint analysis of cluster abundances and auto or cross-correlations of three cosmic tracer fields: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis (4×2pt+N) of cluster abundances, three cluster cross-correlations, and the auto correlations of the galaxy density measured from the first year data of the Dark Energy Survey, we obtain Ω_{m}=0.305_{-0.038}^{+0.055} and σ_{8}=0.783_{-0.054}^{+0.064}. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat νΛCDM model. Consequently, we combine cluster abundances and all two-point correlations from across all three cosmic tracer fields (6×2pt+N) and find improved constraints on cosmological parameters as well as on the cluster observable-mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multiprobe analyses of upcoming wide imaging surveys.
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Affiliation(s)
- C To
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - E Krause
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - E Rozo
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - H Wu
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, Boise State University, Boise, Idaho 83725, USA
| | - D Gruen
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - R H Wechsler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - T F Eifler
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - E S Rykoff
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M Costanzi
- INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy
- Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy
| | - M R Becker
- Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA
| | - G M Bernstein
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - J Blazek
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
| | - S Bocquet
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
| | - S L Bridle
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - R Cawthon
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390
| | - A Choi
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - M Crocce
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - C Davis
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - J DeRose
- Department of Astronomy, University of California, Berkeley, 501 Campbell Hall, Berkeley, California 94720, USA
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - A Drlica-Wagner
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - J Elvin-Poole
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - X Fang
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - A Farahi
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - O Friedrich
- Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - M Gatti
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - E Gaztanaga
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - T Giannantonio
- Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - W G Hartley
- Département de Physique Théorique and Center for Astroparticle Physics, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Geneva, Switzerland
- Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
- Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
| | - B Hoyle
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, 81679 München, Germany
| | - M Jarvis
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - N MacCrann
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - T McClintock
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - V Miranda
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - M E S Pereira
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - Y Park
- Department of Physics, University of Arizona, Tucson, Arizona 85721, USA
| | - A Porredon
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - J Prat
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
| | - M M Rau
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - A J Ross
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - S Samuroff
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - C Sánchez
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - I Sevilla-Noarbe
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - E Sheldon
- Brookhaven National Laboratory, Bldg 510, Upton, New York 11973, USA
| | - M A Troxel
- Department of Physics, Duke University Durham, North Carolina 27708, USA
| | - T N Varga
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, 81679 München, Germany
| | - P Vielzeuf
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - Y Zhang
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J Zuntz
- Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, United Kingdom
| | - T M C Abbott
- Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
| | - M Aguena
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - A Amon
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - J Annis
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S Avila
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - E Bertin
- CNRS, UMR 7095, Institut d'Astrophysique de Paris, F-75014, Paris, France
- Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d'Astrophysique de Paris, F-75014, Paris, France
| | - S Bhargava
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
| | - D Brooks
- Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - D L Burke
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Carnero Rosell
- Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
- Universidad de La Laguna, Dpto. Astrofsica, E-38206 La Laguna, Tenerife, Spain
| | - M Carrasco Kind
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - J Carretero
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - C Chang
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - C Conselice
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
- University of Nottingham, School of Physics and Astronomy, Nottingham NG7 2RD, United Kingdom
| | - L N da Costa
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - T M Davis
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
| | - S Desai
- Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
| | - H T Diehl
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J P Dietrich
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 81679 Munich, Germany
| | - S Everett
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - A E Evrard
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - I Ferrero
- Institute of Theoretical Astrophysics, University of Oslo. P.O. Box 1029 Blindern, NO-0315 Oslo, Norway
| | - B Flaugher
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - P Fosalba
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - J Frieman
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - J García-Bellido
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - R A Gruendl
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - G Gutierrez
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S R Hinton
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
| | - D L Hollowood
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - K Honscheid
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - D Huterer
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D J James
- Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, Massachusetts 02138, USA
| | - T Jeltema
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - R Kron
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - K Kuehn
- Australian Astronomical Optics, Macquarie University, North Ryde, New South Wales 2113, Australia
- Lowell Observatory, 1400 Mars Hill Rd, Flagstaff, Arizona 86001, USA
| | - N Kuropatkin
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - M Lima
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J L Marshall
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - F Menanteau
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - R Miquel
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
- Institució Catalana de Recerca i Estudis Avanćats, E-08010 Barcelona, Spain
| | - R Morgan
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390
| | - J Muir
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - J Myles
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
| | - A Palmese
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - F Paz-Chinchón
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - A A Plazas
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - A K Romer
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
| | - A Roodman
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - E Sanchez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - B Santiago
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Instituto de Física, UFRGS, Caixa Postal 15051, Porto Alegre, RS-91501-970, Brazil
| | - V Scarpine
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S Serrano
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - M Smith
- School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, United Kingdom
| | - E Suchyta
- Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831
| | - M E C Swanson
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - G Tarle
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D Thomas
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - D L Tucker
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J Weller
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr. 1, 81679 München, Germany
| | - W Wester
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - R D Wilkinson
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
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Nadler EO, Drlica-Wagner A, Bechtol K, Mau S, Wechsler RH, Gluscevic V, Boddy K, Pace AB, Li TS, McNanna M, Riley AH, García-Bellido J, Mao YY, Green G, Burke DL, Peter A, Jain B, Abbott TMC, Aguena M, Allam S, Annis J, Avila S, Brooks D, Carrasco Kind M, Carretero J, Costanzi M, da Costa LN, De Vicente J, Desai S, Diehl HT, Doel P, Everett S, Evrard AE, Flaugher B, Frieman J, Gerdes DW, Gruen D, Gruendl RA, Gschwend J, Gutierrez G, Hinton SR, Honscheid K, Huterer D, James DJ, Krause E, Kuehn K, Kuropatkin N, Lahav O, Maia MAG, Marshall JL, Menanteau F, Miquel R, Palmese A, Paz-Chinchón F, Plazas AA, Romer AK, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Soares-Santos M, Suchyta E, Swanson MEC, Tarle G, Tucker DL, Walker AR, Wester W. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies. Phys Rev Lett 2021; 126:091101. [PMID: 33750144 DOI: 10.1103/physrevlett.126.091101] [Citation(s) in RCA: 6] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/30/2020] [Revised: 12/12/2020] [Accepted: 01/27/2021] [Indexed: 06/12/2023]
Abstract
We perform a comprehensive study of Milky Way (MW) satellite galaxies to constrain the fundamental properties of dark matter (DM). This analysis fully incorporates inhomogeneities in the spatial distribution and detectability of MW satellites and marginalizes over uncertainties in the mapping between galaxies and DM halos, the properties of the MW system, and the disruption of subhalos by the MW disk. Our results are consistent with the cold, collisionless DM paradigm and yield the strongest cosmological constraints to date on particle models of warm, interacting, and fuzzy dark matter. At 95% confidence, we report limits on (i) the mass of thermal relic warm DM, m_{WDM}>6.5 keV (free-streaming length, λ_{fs}≲10h^{-1} kpc), (ii) the velocity-independent DM-proton scattering cross section, σ_{0}<8.8×10^{-29} cm^{2} for a 100 MeV DM particle mass [DM-proton coupling, c_{p}≲(0.3 GeV)^{-2}], and (iii) the mass of fuzzy DM, m_{ϕ}>2.9×10^{-21} eV (de Broglie wavelength, λ_{dB}≲0.5 kpc). These constraints are complementary to other observational and laboratory constraints on DM properties.
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Affiliation(s)
- E O Nadler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Drlica-Wagner
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
| | - K Bechtol
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USA
| | - S Mau
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - R H Wechsler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - V Gluscevic
- University of Southern California, Department of Physics and Astronomy, 825 Bloom Walk ACB 439, Los Angeles, California 90089-0484, USA
| | - K Boddy
- Theory Group, Department of Physics, The University of Texas at Austin, Austin, Texas 78712, USA
| | - A B Pace
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - T S Li
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
- Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, California 91101, USA
| | - M McNanna
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue, Madison, Wisconsin 53706-1390, USA
| | - A H Riley
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - J García-Bellido
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - Y-Y Mao
- Department of Physics and Astronomy, Rutgers, The State University of New Jersey, Piscataway, New Jersey 08854, USA
| | - G Green
- Max Planck Institute for Astronomy, Königstuhl 17 D-69117, Heidelberg, Germany
| | - D L Burke
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Peter
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Astronomy, The Ohio State University, Columbus, Ohio 43210, USA
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - B Jain
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - T M C Abbott
- Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
| | - M Aguena
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - S Allam
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - J Annis
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - S Avila
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - D Brooks
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - M Carrasco Kind
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - J Carretero
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), Spain
| | - M Costanzi
- INAF-Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, I-34143 Trieste, Italy
- Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy
| | - L N da Costa
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J De Vicente
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - S Desai
- Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
| | - H T Diehl
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - P Doel
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - S Everett
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - A E Evrard
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - B Flaugher
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - J Frieman
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - D W Gerdes
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D Gruen
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, P.O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - R A Gruendl
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - J Gschwend
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - G Gutierrez
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - S R Hinton
- School of Mathematics and Physics, University of Queensland, Brisbane, Queensland 4072, Australia
| | - K Honscheid
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - D Huterer
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D J James
- Center for Astrophysics, Harvard and Smithsonian, 60 Garden Street, Cambridge, Massachusetts 02138, USA
| | - E Krause
- Department of Astronomy/Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
| | - K Kuehn
- Australian Astronomical Optics, Macquarie University, North Ryde, New South Wales 2113, Australia
- Lowell Observatory, 1400 Mars Hill Road, Flagstaff, Arizona 86001, USA
| | - N Kuropatkin
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - O Lahav
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J L Marshall
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - F Menanteau
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - R Miquel
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona), Spain
- Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
| | - A Palmese
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - F Paz-Chinchón
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - A A Plazas
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - A K Romer
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton, BN1 9QH, United Kingdom
| | - E Sanchez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - V Scarpine
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - S Serrano
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - I Sevilla-Noarbe
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - M Smith
- School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, United Kingdom
| | - M Soares-Santos
- Brandeis University, Physics Department, 415 South Street, Waltham, Massachusetts 02453, USA
| | - E Suchyta
- Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - M E C Swanson
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - G Tarle
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D L Tucker
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
| | - A R Walker
- Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, Casilla 603, La Serena, Chile
| | - W Wester
- Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510, USA
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Costanzi M, Saro A, Bocquet S, Abbott T, Aguena M, Allam S, Amara A, Annis J, Avila S, Bacon D, Benson B, Bhargava S, Brooks D, Buckley-Geer E, Burke D, Carnero Rosell A, Carrasco Kind M, Carretero J, Choi A, da Costa L, Pereira M, De Vicente J, Desai S, Diehl H, Dietrich J, Doel P, Eifler T, Everett S, Ferrero I, Ferté A, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Giles P, Grandis S, Gruen D, Gruendl R, Gupta N, Gutierrez G, Hartley W, Hinton S, Hollowood D, Honscheid K, James D, Jeltema T, Krause E, Kuehn K, Kuropatkin N, Lahav O, Lima M, MacCrann N, Maia M, Marshall J, Menanteau F, Miquel R, Mohr J, Morgan R, Myles J, Ogando R, Palmese A, Paz-Chinchón F, Plazas A, Rapetti D, Reichardt C, Romer A, Roodman A, Ruppin F, Salvati L, Samuroff S, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Singh P, Smith M, Soares-Santos M, Stark A, Suchyta E, Swanson M, Tarle G, Thomas D, To C, Tucker D, Varga T, Wechsler R, Zhang Z. Cosmological constraints from DES Y1 cluster abundances and SPT multiwavelength data. Int J Clin Exp Med 2021. [DOI: 10.1103/physrevd.103.043522] [Citation(s) in RCA: 17] [Impact Index Per Article: 5.7] [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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Muir J, Baxter E, Miranda V, Doux C, Ferté A, Leonard C, Huterer D, Jain B, Lemos P, Raveri M, Nadathur S, Campos A, Chen A, Dodelson S, Elvin-Poole J, Lee S, Secco L, Troxel M, Weaverdyck N, Zuntz J, Brout D, Choi A, Crocce M, Davis T, Gruen D, Krause E, Lidman C, MacCrann N, Möller A, Prat J, Ross A, Sako M, Samuroff S, Sánchez C, Scolnic D, Zhang B, Abbott T, Aguena M, Allam S, Annis J, Avila S, Bacon D, Bertin E, Bhargava S, Bridle S, Brooks D, Burke D, Carnero Rosell A, Carrasco Kind M, Carretero J, Cawthon R, Costanzi M, da Costa L, Pereira M, Desai S, Diehl H, Dietrich J, Doel P, Estrada J, Everett S, Evrard A, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Giannantonio T, Gruendl R, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, Hoyle B, James D, Jeltema T, Kuehn K, Kuropatkin N, Lahav O, Lima M, Maia M, Menanteau F, Miquel R, Morgan R, Myles J, Palmese A, Paz-Chinchón F, Plazas A, Romer A, Roodman A, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Suchyta E, Swanson M, Tarle G, Thomas D, To C, Tucker D, Varga T, Weller J, Wilkinson R. DES Y1 results: Splitting growth and geometry to test
ΛCDM. Int J Clin Exp Med 2021. [DOI: 10.1103/physrevd.103.023528] [Citation(s) in RCA: 10] [Impact Index Per Article: 3.3] [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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Jafari L, Doerr O, Chelladurai P, Pullamsetti S, Troidl C, Keller T, Guenther S, Gruen D, Keranov S, Kriechbaum S, Liebetrau C, Mayer E, Seeger W, Hamm C, Nef H. Shift in transcriptional landscape of human right ventricle in chronic thromboembolic pulmonary arterial hypertension. Eur Heart J 2020. [DOI: 10.1093/ehjci/ehaa946.2230] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
Abstract
Abstract
Background
Chronic thromboembolic pulmonary hypertension (CTEPH) is a sub group of pulmonary hypertension (PH). CTEPH is characterized by the existence of thromboemboli and vascular remodeling in pulmonary vessels. The effect of increase in pulmonary artery pressures causes right ventricle (RV) hypertrophy and dilatation and finally leads to right heart failure and death. Surgical intervention in operable patients makes the CTEPH as an only curable and unique form of ph. Pulmonary endarterectomy (PEA) is the surgical procedure to remove the thromboembolic clots from the pulmonary vasculature, which restores RV function back to normal with significant improvements in cardiovascular magnetic resonance.
Purpose
The aim of this study is to use transcriptomic profiling to identify signaling pathways, master regulators, and potentially new biomarkers that specifically indicate the effect of PEA on the RV of patients with chronic thromboembolic pulmonary hypertension.
Results
RNA -sequencing (RNA-seq) was performed on RV biopsies obtained from CTEPH patients at PEA baseline (before PEA surgery) and the results were compared with those from RV biopsies obtained during follow-up evaluation. Bioinformatic analysis of RNA-seq data identified 2799 genes (n=14, −0.585 ≤ Log2 fold change ≥0.585, FDR ≤0.05) differentially regulated between the PEA baseline and follow-up sample groups. The great number of genes (2799) differentially expressed after PEA surgery in CTEPH patients confirms a major shift in the transcriptional landscape of RV in these patients. To further identify potential biomarker candidates from the large pool of 2799 differentially expressed genes (DEGs), extensive bioinformatic analysis of different data sets shortlisted 250 DEGs that were functionally associated with cardiovascular development or disease. The findings of this study reveal prominent transcriptional changes that occur in response to PEA. Gene ontology enrichment and pathway analysis confirmed altered regulation of hypoxia-inducible factor 1 (HIF-1) signaling, advanced glycation end products and their receptors (AGE-RAGE), mitogen-activated protein kinase (MAPK) signaling, hippo signaling, the Janus kinase/ signal transducers and activators of transcription (Jak-STAT) signaling pathway, and proteoglycans after PEA compared with before PEA.
Conclusion
Comparison of the results of RNA-seq analysis of RV biopsies of CTEPH patients, pre and post PEA, revealed a major shift in the transcriptional landscape of these patients after reducing the pressure overload of the RV by PEA.
Funding Acknowledgement
Type of funding source: Foundation. Main funding source(s): German Research Foundation (DFG)
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Affiliation(s)
- L Jafari
- Justus-Liebig University of Giessen, Giessen, Germany
| | - O Doerr
- University hospital Giessen and Marburg, Medical Clinic I, Department of Cardiology and Angiology, Giessen, Germany
| | - P Chelladurai
- Max Planck Institute for Heart and Lung Research, Department of lung Development and Remodeling, Bad Nauheim, Germany
| | - S.S Pullamsetti
- Max Planck Institute for Heart and Lung Research, Department of lung Development and Remodeling, Bad Nauheim, Germany
| | - C Troidl
- Justus-Liebig University of Giessen, Giessen, Germany
| | - T Keller
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - S Guenther
- Max Planck Institute for Heart and Lung Research, Bioinformatics and deep sequencing platform, Bad Nauheim, Germany
| | - D Gruen
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - S Keranov
- University hospital Giessen and Marburg, Medical Clinic I, Department of Cardiology and Angiology, Giessen, Germany
| | - S Kriechbaum
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - C Liebetrau
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - E Mayer
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - W Seeger
- University Hospital Giessen and Marburg, Medical Clinic II – Pneumology, Giessen, Germany
| | - C.W Hamm
- University hospital Giessen and Marburg, Medical Clinic I, Department of Cardiology and Angiology, Giessen, Germany
| | - H.M Nef
- University hospital Giessen and Marburg, Medical Clinic I, Department of Cardiology and Angiology, Giessen, Germany
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Abbott T, Aguena M, Alarcon A, Allam S, Allen S, Annis J, Avila S, Bacon D, Bechtol K, Bermeo A, Bernstein G, Bertin E, Bhargava S, Bocquet S, Brooks D, Brout D, Buckley-Geer E, Burke D, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Cawthon R, Chang C, Chen X, Choi A, Costanzi M, Crocce M, da Costa L, Davis T, De Vicente J, DeRose J, Desai S, Diehl H, Dietrich J, Dodelson S, Doel P, Drlica-Wagner A, Eckert K, Eifler T, Elvin-Poole J, Estrada J, Everett S, Evrard A, Farahi A, Ferrero I, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gatti M, Gaztanaga E, Gerdes D, Giannantonio T, Giles P, Grandis S, Gruen D, Gruendl R, Gschwend J, Gutierrez G, Hartley W, Hinton S, Hollowood D, Honscheid K, Hoyle B, Huterer D, James D, Jarvis M, Jeltema T, Johnson M, Johnson M, Kent S, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Li T, Lidman C, Lima M, Lin H, MacCrann N, Maia M, Mantz A, Marshall J, Martini P, Mayers J, Melchior P, Mena-Fernández J, Menanteau F, Miquel R, Mohr J, Nichol R, Nord B, Ogando R, Palmese A, Paz-Chinchón F, Plazas A, Prat J, Rau M, Romer A, Roodman A, Rooney P, Rozo E, Rykoff E, Sako M, Samuroff S, Sánchez C, Sanchez E, Saro A, Scarpine V, Schubnell M, Scolnic D, Serrano S, Sevilla-Noarbe I, Sheldon E, Smith J, Smith M, Suchyta E, Swanson M, Tarle G, Thomas D, To C, Troxel M, Tucker D, Varga T, von der Linden A, Walker A, Wechsler R, Weller J, Wilkinson R, Wu H, Yanny B, Zhang Y, Zhang Z, Zuntz J. Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing. Int J Clin Exp Med 2020. [DOI: 10.1103/physrevd.102.023509] [Citation(s) in RCA: 98] [Impact Index Per Article: 24.5] [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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Kacprzak T, Herbel J, Nicola A, Sgier R, Tarsitano F, Bruderer C, Amara A, Refregier A, Bridle S, Drlica-Wagner A, Gruen D, Hartley W, Hoyle B, Secco L, Zuntz J, Annis J, Avila S, Bertin E, Brooks D, Buckley-Geer E, Carnero Rosell A, Carrasco Kind M, Carretero J, da Costa L, De Vicente J, Desai S, Diehl H, Doel P, García-Bellido J, Gaztanaga E, Gruendl R, Gschwend J, Gutierrez G, Hollowood D, Honscheid K, James D, Jarvis M, Lima M, Maia M, Marshall J, Melchior P, Menanteau F, Miquel R, Paz-Chinchón F, Plazas A, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Suchyta E, Swanson M, Tarle G, Vikram V, Weller J. Monte Carlo control loops for cosmic shear cosmology with DES Year 1 data. Int J Clin Exp Med 2020. [DOI: 10.1103/physrevd.101.082003] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.0] [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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18
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Ammazzalorso S, Gruen D, Regis M, Camera S, Ando S, Fornengo N, Bechtol K, Bridle SL, Choi A, Eifler TF, Gatti M, MacCrann N, Omori Y, Samuroff S, Sheldon E, Troxel MA, Zuntz J, Carrasco Kind M, Annis J, Avila S, Bertin E, Brooks D, Burke DL, Carnero Rosell A, Carretero J, Castander FJ, Costanzi M, da Costa LN, De Vicente J, Desai S, Diehl HT, Dietrich JP, Doel P, Everett S, Flaugher B, Fosalba P, García-Bellido J, Gaztanaga E, Gerdes DW, Giannantonio T, Goldstein DA, Gruendl RA, Gutierrez G, Hollowood DL, Honscheid K, James DJ, Jarvis M, Jeltema T, Kent S, Kuropatkin N, Lahav O, Li TS, Lima M, Maia MAG, Marshall JL, Melchior P, Menanteau F, Miquel R, Ogando RLC, Palmese A, Plazas AA, Romer AK, Roodman A, Rykoff ES, Sánchez C, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thomas D, Vikram V, Zhang Y. Detection of Cross-Correlation between Gravitational Lensing and γ Rays. Phys Rev Lett 2020; 124:101102. [PMID: 32216401 DOI: 10.1103/physrevlett.124.101102] [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: 08/22/2019] [Revised: 12/14/2019] [Accepted: 01/13/2020] [Indexed: 06/10/2023]
Abstract
In recent years, many γ-ray sources have been identified, yet the unresolved component hosts valuable information on the faintest emission. In order to extract it, a cross-correlation with gravitational tracers of matter in the Universe has been shown to be a promising tool. We report here the first identification of a cross-correlation signal between γ rays and the distribution of mass in the Universe probed by weak gravitational lensing. We use data from the Dark Energy Survey Y1 weak lensing data and the Fermi Large Area Telescope 9-yr γ-ray data, obtaining a signal-to-noise ratio of 5.3. The signal is mostly localized at small angular scales and high γ-ray energies, with a hint of correlation at extended separation. Blazar emission is likely the origin of the small-scale effect. We investigate implications of the large-scale component in terms of astrophysical sources and particle dark matter emission.
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Affiliation(s)
- S Ammazzalorso
- Dipartimento di Fisica, Università degli Studi di Torino, via Pietro Giuria 1, 10125 Torino, Italy
- INFN-Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via Pietro Giuria 1, 10125 Torino, Italy
| | - D Gruen
- Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M Regis
- Dipartimento di Fisica, Università degli Studi di Torino, via Pietro Giuria 1, 10125 Torino, Italy
- INFN-Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via Pietro Giuria 1, 10125 Torino, Italy
| | - S Camera
- Dipartimento di Fisica, Università degli Studi di Torino, via Pietro Giuria 1, 10125 Torino, Italy
- INFN-Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via Pietro Giuria 1, 10125 Torino, Italy
- INAF-Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Torino, strada Osservatorio 20, 10025 Pino Torinese, Italy
- Department of Physics and Astronomy, University of the Western Cape, Cape Town 7535, South Africa
| | - S Ando
- GRAPPA Institute, University of Amsterdam, 1098 XH Amsterdam, The Netherlands
- Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - N Fornengo
- Dipartimento di Fisica, Università degli Studi di Torino, via Pietro Giuria 1, 10125 Torino, Italy
- INFN-Istituto Nazionale di Fisica Nucleare, Sezione di Torino, via Pietro Giuria 1, 10125 Torino, Italy
| | - K Bechtol
- LSST, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390, USA
| | - S L Bridle
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, United Kingdom
| | - A Choi
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - T F Eifler
- Department of Astronomy and Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - M Gatti
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra, Barcelona, Spain
| | - N MacCrann
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - Y Omori
- Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - S Samuroff
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - E Sheldon
- Brookhaven National Laboratory, Building 510, Upton, New York 11973, USA
| | - M A Troxel
- Department of Physics, Duke University Durham, North Carolina 27708, USA
| | - J Zuntz
- Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, United Kingdom
| | - M Carrasco Kind
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - J Annis
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S Avila
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - E Bertin
- CNRS, UMR 7095, Institut d'Astrophysique de Paris, F-75014 Paris, France
- Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d'Astrophysique de Paris, F-75014 Paris, France
| | - D Brooks
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - D L Burke
- Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - A Carnero Rosell
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J Carretero
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra, Barcelona, Spain
| | - F J Castander
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - M Costanzi
- INAF-Osservatorio Astronomico di Trieste, via Giambattista Tiepolo 11, 34143 Trieste, Italy
- IFPU-Institute for Fundamental Physics of the Universe, Via Beirut 2, 34014 Trieste, Italy
| | - L N da Costa
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J De Vicente
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain
| | - S Desai
- Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
| | - H T Diehl
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J P Dietrich
- Excellence Cluster Origins, Boltzmannstrasse 2, 85748 Garching, Germany
- Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstrasse 1, 81679 Munich, Germany
| | - P Doel
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - S Everett
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - B Flaugher
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - P Fosalba
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - J García-Bellido
- Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - E Gaztanaga
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - D W Gerdes
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - T Giannantonio
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - D A Goldstein
- California Institute of Technology, 1200 East California Boulevard, MC 249-17, Pasadena, California 91125, USA
| | - R A Gruendl
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - G Gutierrez
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - D L Hollowood
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - K Honscheid
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - D J James
- Center for Astrophysics, Harvard-Smithsonian, 60 Garden Street, Cambridge, Massachusetts 02138, USA
| | - M Jarvis
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - T Jeltema
- Santa Cruz Institute for Particle Physics, Santa Cruz, California 95064, USA
| | - S Kent
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - N Kuropatkin
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - O Lahav
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - T S Li
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - M Lima
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP, 05314-970, Brazil
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - J L Marshall
- George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA
| | - P Melchior
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - F Menanteau
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - R Miquel
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra, Barcelona, Spain
- Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
| | - R L C Ogando
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Observatório Nacional, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
| | - A Palmese
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - A A Plazas
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - A K Romer
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, United Kingdom
| | - A Roodman
- Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - E S Rykoff
- Kavli Institute for Particle Astrophysics and Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C Sánchez
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - E Sanchez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain
| | - V Scarpine
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - S Serrano
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - I Sevilla-Noarbe
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain
| | - M Smith
- School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - M Soares-Santos
- Brandeis University, Physics Department, 415 South Street, Waltham, Massachusetts 02453, USA
| | - F Sobreira
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General José Cristino 77, Rio de Janeiro, RJ-20921-400, Brazil
- Instituto de Física Gleb Wataghin, Universidade Estadual de Campinas, 13083-859 Campinas, São Paulo, Brazil
| | - E Suchyta
- Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - M E C Swanson
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - G Tarle
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - D Thomas
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - V Vikram
- Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA
| | - Y Zhang
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
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19
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Elsner LK, Pilz S, Von Jeinsen B, Diouf K, Wolter JS, Gruen D, Kleber M, Drechsler C, Troidl C, Doerr O, Wanner C, Hamm CW, Liebetrau C, Maerz W, Keller T. P5478Information on weather conditions improves the prognostic ability of 25 OH-vitamin D in stable coronary artery disease. Eur Heart J 2019. [DOI: 10.1093/eurheartj/ehz746.0432] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
Abstract
Abstract
Introduction and aim
Vitamin D deficiency is associated with an adverse prognosis in patients with coronary artery disease (CAD). Decreased levels of vitamin D are associated with low sunshine exposure, resulting in seasonal variations of vitamin D. The aims of this study were to investigate the influence of different specific weather conditions on vitamin D levels and to explore a possible improvement of risk stratification by vitamin D levels in stable patients with CAD using meteorological data.
Methods
The study population consists of two independent cohorts of stable patients undergoing coronary angiography with suspected or known CAD: as derivation cohort, the ongoing biomarker registry BioPROSPECTIVE with n=1,766 enrolled patients between 2010 and 2013 (median age 70.1 yrs; 30.8% females); and as validation cohort, the Ludwigshafen Risk and Cardiovascular Health (LURIC) Study with n=3,299 patients (median age 63.5 yrs; 30.3% females). In the derivation cohort 235 (13.3%) patients were known to be deceased by 08/2018. In the validation cohort 760 (23.0%) patients died within a median follow-up time of 7.75 years. 25-OH vitamin D levels were measured by commercial assays. Vitamin D deficiency was defined as 25-OH vitamin D levels ≤20 ng/mL. Daily averaged data on six weather conditions of the 180 days prior to enrolment were collected for each patient from the weather station located closest to the respective study centre. Using air pressure, precipitation height, sunshine duration, temperature, relative humidity, and vapour pressure a weather model was constructed that significantly correlated with vitamin D levels (r=0.37; p<0.001).
Results
In the derivation cohort, median vitamin D levels were lower in non-survivors (13.3 [9.65–19.65] ng/mL) than in survivors (15.70 [10.7–22.65] ng/mL; p<0.001). Vitamin D predicted all-cause mortality with an area under the receiver operator characteristic curve (AUROC) of 0.576 (CI: 0.54–0.62). Adding the weather model to vitamin D significantly improved the AUROC to 0.601 (CI: 0.56–0.64; p=0.031). The vitamin D/weather model combination enhanced the prognostic value of the ESC SCORE to predict mortality (AUROC=0.571 [CI: 0.53–0.61] vs. 0.628 [CI: 0.59–0.67]; p=0.004). Comparable results were observed in the validation cohort. Here, vitamin D deficiency predicted mortality with a hazard ratio (HR) of 1.89 (CI: 1.59–2.26) after adjustment for ESC SCORE. Adding the weather model improved this HR to 1.92 (1.62–2.32). Reclassification analyses support the additive prognostic information of weather conditions with a continuous net reclassification improvement of 0.114 ([0.033–0.194]; p=0.006) if adding the weather model to vitamin D as base model for predicting mortality.
Conclusions
Different weather conditions show a significant impact on vitamin D levels in stable patients. Adding data on weather conditions improve the risk stratification by vitamin D for predicting mortality in stable CAD patients.
Acknowledgement/Funding
The study is financially supported by the Kerckhoff Heart Research Institute (KHFI) and the German Center for Cardiovascular Research (DZHK).
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Affiliation(s)
- L K Elsner
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - S Pilz
- Medical University of Graz, Department of Internal Medicine, Division of Endocrinology and Diabetology, Graz, Austria
| | - B Von Jeinsen
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - K Diouf
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - J S Wolter
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - D Gruen
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - M Kleber
- University Medical Centre of Mannheim, Vth Department of Medicine (Nephrology, Hypertensiology, Endocrinology, Diabetology, Rheumatology), Mannheim, Germany
| | - C Drechsler
- University of Wuerzburg, Department of Medicine I, Division of Nephrology, Wurzburg, Germany
| | - C Troidl
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - O Doerr
- Justus-Liebig University of Giessen, Department of Cardiology, Giessen, Germany
| | - C Wanner
- University of Wuerzburg, Department of Medicine I, Division of Nephrology, Wurzburg, Germany
| | - C W Hamm
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - C Liebetrau
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
| | - W Maerz
- University Medical Centre of Mannheim, Vth Department of Medicine (Nephrology, Hypertensiology, Endocrinology, Diabetology, Rheumatology), Mannheim, Germany
| | - T Keller
- Kerckhoff Heart and Thorax Center, Department of Cardiology, Bad Nauheim, Germany
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20
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Omori Y, Baxter E, Chang C, Kirk D, Alarcon A, Bernstein G, Bleem L, Cawthon R, Choi A, Chown R, Crawford T, Davis C, De Vicente J, DeRose J, Dodelson S, Eifler T, Fosalba P, Friedrich O, Gatti M, Gaztanaga E, Giannantonio T, Gruen D, Hartley W, Holder G, Hoyle B, Huterer D, Jain B, Jarvis M, Krause E, MacCrann N, Miquel R, Prat J, Rau M, Reichardt C, Rozo E, Samuroff S, Sánchez C, Secco L, Sheldon E, Simard G, Troxel M, Vielzeuf P, Wechsler R, Zuntz J, Abbott T, Abdalla F, Allam S, Annis J, Avila S, Aylor K, Benson B, Bertin E, Bridle S, Brooks D, Burke D, Carlstrom J, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Chang C, Cho HM, Crites A, Crocce M, Cunha C, da Costa L, de Haan T, Desai S, Diehl H, Dietrich J, Dobbs M, Everett W, Fernandez E, Flaugher B, Frieman J, García-Bellido J, George E, Gruendl R, Gutierrez G, Halverson N, Harrington N, Hollowood D, Honscheid K, Holzapfel W, Hou Z, Hrubes J, James D, Jeltema T, Kuehn K, Kuropatkin N, Lima M, Lin H, Lee A, Leitch E, Luong-Van D, Maia M, Manzotti A, Marrone D, Marshall J, Martini P, McMahon J, Melchior P, Menanteau F, Meyer S, Mocanu L, Mohr J, Natoli T, Ogando R, Padin S, Plazas A, Pryke C, Romer A, Roodman A, Ruhl J, Rykoff E, Sanchez E, Scarpine V, Schaffer K, Schindler R, Sevilla-Noarbe I, Shirokoff E, Smith M, Smith R, Soares-Santos M, Sobreira F, Staniszewski Z, Stark A, Story K, Suchyta E, Swanson M, Tarle G, Thomas D, Vanderlinde K, Vieira J, Vikram V, Walker A, Weller J, Williamson R, Wu W, Zahn O. Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope
+Planck
CMB weak lensing. Int J Clin Exp Med 2019. [DOI: 10.1103/physrevd.100.043517] [Citation(s) in RCA: 12] [Impact Index Per Article: 2.4] [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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21
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Abbott TMC, Alarcon A, Allam S, Andersen P, Andrade-Oliveira F, Annis J, Asorey J, Avila S, Bacon D, Banik N, Bassett BA, Baxter E, Bechtol K, Becker MR, Bernstein GM, Bertin E, Blazek J, Bridle SL, Brooks D, Brout D, Burke DL, Calcino J, Camacho H, Campos A, Carnero Rosell A, Carollo D, Carrasco Kind M, Carretero J, Castander FJ, Cawthon R, Challis P, Chan KC, Chang C, Childress M, Crocce M, Cunha CE, D'Andrea CB, da Costa LN, Davis C, Davis TM, De Vicente J, DePoy DL, DeRose J, Desai S, Diehl HT, Dietrich JP, Dodelson S, Doel P, Drlica-Wagner A, Eifler TF, Elvin-Poole J, Estrada J, Evrard AE, Fernandez E, Flaugher B, Foley RJ, Fosalba P, Frieman J, Galbany L, García-Bellido J, Gatti M, Gaztanaga E, Gerdes DW, Giannantonio T, Glazebrook K, Goldstein DA, Gruen D, Gruendl RA, Gschwend J, Gutierrez G, Hartley WG, Hinton SR, Hollowood DL, Honscheid K, Hoormann JK, Hoyle B, Huterer D, Jain B, James DJ, Jarvis M, Jeltema T, Kasai E, Kent S, Kessler R, Kim AG, Kokron N, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Lasker J, Lemos P, Lewis GF, Li TS, Lidman C, Lima M, Lin H, Macaulay E, MacCrann N, Maia MAG, March M, Marriner J, Marshall JL, Martini P, McMahon RG, Melchior P, Menanteau F, Miquel R, Mohr JJ, Morganson E, Muir J, Möller A, Neilsen E, Nichol RC, Nord B, Ogando RLC, Palmese A, Pan YC, Peiris HV, Percival WJ, Plazas AA, Porredon A, Prat J, Romer AK, Roodman A, Rosenfeld R, Ross AJ, Rykoff ES, Samuroff S, Sánchez C, Sanchez E, Scarpine V, Schindler R, Schubnell M, Scolnic D, Secco LF, Serrano S, Sevilla-Noarbe I, Sharp R, Sheldon E, Smith M, Soares-Santos M, Sobreira F, Sommer NE, Swann E, Swanson MEC, Tarle G, Thomas D, Thomas RC, Troxel MA, Tucker BE, Uddin SA, Vielzeuf P, Walker AR, Wang M, Weaverdyck N, Wechsler RH, Weller J, Yanny B, Zhang B, Zhang Y, Zuntz J. Cosmological Constraints from Multiple Probes in the Dark Energy Survey. Phys Rev Lett 2019; 122:171301. [PMID: 31107093 DOI: 10.1103/physrevlett.122.171301] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/08/2018] [Revised: 02/19/2019] [Indexed: 06/09/2023]
Abstract
The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically confirmed type Ia supernova light curves, the baryon acoustic oscillation feature, weak gravitational lensing, and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, w, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave background, the probes from this single photometric survey rule out a Universe with no dark energy, finding w=-0.80_{-0.11}^{+0.09}. The geometry is shown to be consistent with a spatially flat Universe, and we obtain a constraint on the baryon density of Ω_{b}=0.069_{-0.012}^{+0.009} that is independent of early Universe measurements. These results demonstrate the potential power of large multiprobe photometric surveys and pave the way for order of magnitude advances in our constraints on properties of dark energy and cosmology over the next decade.
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Affiliation(s)
- T M C Abbott
- Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
| | - A Alarcon
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - S Allam
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - P Andersen
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
- University of Copenhagen, Dark Cosmology Centre, Juliane Maries Vej 30, 2100 Copenhagen O, Denmark
| | - F Andrade-Oliveira
- Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, Brazil
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - J Annis
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J Asorey
- Korea Astronomy and Space Science Institute, Yuseong-gu, Daejeon 305-348, Korea
| | - S Avila
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - D Bacon
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - N Banik
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - B A Bassett
- African Institute for Mathematical Sciences, 6 Melrose Road, Muizenberg 7945, South Africa
- South African Astronomical Observatory, P.O.Box 9, Observatory 7935, South Africa
| | - E Baxter
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - K Bechtol
- LSST, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390, USA
| | - M R Becker
- Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA
| | - G M Bernstein
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - E Bertin
- CNRS, UMR 7095, Institut d'Astrophysique de Paris, F-75014 Paris, France
- Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d'Astrophysique de Paris, F-75014 Paris, France
| | - J Blazek
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Institute of Physics, Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
| | - S L Bridle
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - D Brooks
- Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - D Brout
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - D L Burke
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - J Calcino
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
| | - H Camacho
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, Brazil
| | - A Campos
- Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, Brazil
- Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
| | - A Carnero Rosell
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - D Carollo
- INAF, Astrophysical Observatory of Turin, I-10025 Pino Torinese, Italy
| | - M Carrasco Kind
- Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark St., Urbana, Illinois 61801, USA
| | - J Carretero
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
| | - F J Castander
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - R Cawthon
- Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison, 1150 University Avenue Madison, Wisconsin 53706-1390, USA
| | - P Challis
- Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, Massachusetts 02138, USA
| | - K C Chan
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - C Chang
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - M Childress
- School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - M Crocce
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
- Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
| | - C E Cunha
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - C B D'Andrea
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - L N da Costa
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - C Davis
- Kavli Institute for Particle Astrophysics & Cosmology, P. O. Box 2450, Stanford University, Stanford, California 94305, USA
| | - T M Davis
- School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
| | - J De Vicente
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
| | - D L DePoy
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| | - S Desai
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| | - H T Diehl
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| | - J P Dietrich
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| | - J Elvin-Poole
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| | - E Gaztanaga
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| | - K Glazebrook
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| | - R A Gruendl
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| | - J Gschwend
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| | - W G Hartley
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| | - S R Hinton
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| | - K Honscheid
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| | - B Hoyle
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| | - S Kent
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| | - A G Kim
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| | - N Kokron
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| | - E Krause
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| | - R Kron
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| | - K Kuehn
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| | - N Kuropatkin
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| | - O Lahav
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| | - G F Lewis
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| | - T S Li
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| | - C Lidman
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| | - M Lima
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| | - H Lin
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| | - E Macaulay
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| | - N MacCrann
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- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
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- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - J Marriner
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| | - R G McMahon
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| | - F Menanteau
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| | - R Miquel
- Institut de Física d'Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra (Barcelona) Spain
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| | - J J Mohr
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| | - E Neilsen
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| | - B Nord
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| | - R L C Ogando
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
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| | - A Palmese
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| | - Y-C Pan
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| | - W J Percival
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| | - A A Plazas
- Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA
| | - A Porredon
- Institut d'Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
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| | - J Prat
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| | - A K Romer
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| | - A J Ross
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| | - E S Rykoff
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| | - S Samuroff
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| | - E Sanchez
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| | - V Scarpine
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| | - D Scolnic
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| | - S Serrano
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| | - I Sevilla-Noarbe
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| | - R Sharp
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| | - M Soares-Santos
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| | - F Sobreira
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| | - N E Sommer
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| | - D Thomas
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| | - R C Thomas
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- Department of Physics, Duke University, Durham, North Carolina 27708, USA
| | - B E Tucker
- The Research School of Astronomy and Astrophysics, Australian National University, ACT 2601, Australia
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| | - S A Uddin
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| | - A R Walker
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| | - M Wang
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| | - N Weaverdyck
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| | - R H Wechsler
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| | - J Weller
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| | - B Yanny
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| | - B Zhang
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| | - Y Zhang
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| | - J Zuntz
- Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, United Kingdom
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Affiliation(s)
- F. Cafasso
- Argonne National Laboratory 9700 South Cass Avenue, Argonne, Illinois 60439
| | - D. Gruen
- Argonne National Laboratory 9700 South Cass Avenue, Argonne, Illinois 60439
| | - M. Kaminsky
- Argonne National Laboratory 9700 South Cass Avenue, Argonne, Illinois 60439
| | - J. E. Robinson
- Argonne National Laboratory 9700 South Cass Avenue, Argonne, Illinois 60439
| | - H. Wiedersich
- Argonne National Laboratory 9700 South Cass Avenue, Argonne, Illinois 60439
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Lopes JC, de Matos LF, Harper MT, Giallongo F, Oh J, Gruen D, Ono S, Kindermann M, Duval S, Hristov AN. Effect of 3-nitrooxypropanol on methane and hydrogen emissions, methane isotopic signature, and ruminal fermentation in dairy cows. J Dairy Sci 2016; 99:5335-5344. [PMID: 27085412 DOI: 10.3168/jds.2015-10832] [Citation(s) in RCA: 72] [Impact Index Per Article: 9.0] [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: 12/28/2015] [Accepted: 03/08/2016] [Indexed: 11/19/2022]
Abstract
The objective of this crossover experiment was to investigate the effect of a methane inhibitor, 3-nitrooxypropanol (3NOP), on enteric methane emission, methane isotopic composition, and rumen fermentation and microbial profile in lactating dairy cows. The experiment involved 6 ruminally cannulated late-lactation Holstein cows assigned to 2 treatments: control and 3NOP (60 mg/kg of feed dry matter). Compared with the control, 3NOP decreased methane emission by 31% and increased hydrogen emission from undetectable to 1.33 g/d. Methane emissions per kilogram of dry matter intake and milk yield were also decreased 34% by 3NOP. Milk production and composition were not affected by 3NOP, except milk fat concentration was increased compared with the control. Concentrations of total VFA and propionate in ruminal fluid were not affected by treatment, but acetate concentration tended to be lower and acetate-to-propionate ratio was lower for 3NOP compared with the control. The 3NOP decreased the molar proportion of acetate and increase those of propionate, butyrate, valerate, and isovalerate. Deuterium-to-hydrogen ratios of methane and the abundance of (13)CH3D were similar between treatments. Compared with the control, minor (4‰) depletion in the (13)C/(12)C ratio was observed for 3NOP. Genus composition of methanogenic archaea (Methanobrevibacter, Methanosphaera, and Methanomicrobium) was not affected by 3NOP, but the proportion of methanogens in the total cell counts tended to be decreased by 3NOP. Prevotella spp., the predominant bacterial genus in ruminal contents in this experiment, was also not affected by 3NOP. Compared with the control, Ruminococcus and Clostridium spp. were decreased and Butyrivibrio spp. was increased by 3NOP. This experiment demonstrated that a substantial inhibition of enteric methane emission by 3NOP in dairy cows was accompanied with increased hydrogen emission and decreased acetate-to-propionate ratio; however, neither an effect on rumen archaeal community composition nor a significant change in the isotope composition of methane was observed.
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Affiliation(s)
- J C Lopes
- Department of Animal Science, The Pennsylvania State University, University Park 16802
| | - L F de Matos
- Department of Animal Science, The Pennsylvania State University, University Park 16802
| | - M T Harper
- Department of Animal Science, The Pennsylvania State University, University Park 16802
| | - F Giallongo
- Department of Animal Science, The Pennsylvania State University, University Park 16802
| | - J Oh
- Department of Animal Science, The Pennsylvania State University, University Park 16802
| | - D Gruen
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge 02139
| | - S Ono
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge 02139
| | - M Kindermann
- DSM Nutritional Products, Animal Nutrition and Health, Basel, Switzerland CH-4002
| | - S Duval
- DSM Nutritional Products France, Research Centre for Animal Nutrition and Health, Saint Louis Cedex, France 68305
| | - A N Hristov
- Department of Animal Science, The Pennsylvania State University, University Park 16802.
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Kessler R, Marriner J, Childress M, Covarrubias R, D’Andrea CB, Finley DA, Fischer J, Foley RJ, Goldstein D, Gupta RR, Kuehn K, Marcha M, Nichol RC, Papadopoulos A, Sako M, Scolnic D, Smith M, Sullivan M, Wester W, Yuan F, Abbott T, Abdalla FB, Allam S, Benoit-Lévy A, Bernstein GM, Bertin E, Brooks D, Rosell AC, Kind MC, Castander FJ, Crocce M, Costa LND, Desai S, Diehl HT, Eifler TF, Neto AF, Flaugher B, Frieman J, Gerdes DW, Gruen D, Gruendl RA, Honscheid K, James DJ, Kuropatkin N, Li TS, Maia MAG, Marshall JL, Martini P, Miller CJ, Miquel R, Nord B, Ogando R, Plazas AA, Reil K, Romer AK, Roodman A, Sanchez E, Sevilla-Noarbe I, Smith RC, Soares-Santos M, Sobreira F, Tarle G, Thaler J, Thomas RC, Tucker D, Walker AR. THE DIFFERENCE IMAGING PIPELINE FOR THE TRANSIENT SEARCH IN THE DARK ENERGY SURVEY. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-6256/150/6/172] [Citation(s) in RCA: 106] [Impact Index Per Article: 11.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Goldstein DA, D’Andrea CB, Fischer JA, Foley RJ, Gupta RR, Kessler R, Kim AG, Nichol RC, Nugent PE, Papadopoulos A, Sako M, Smith M, Sullivan M, Thomas RC, Wester W, Wolf RC, Abdalla FB, Banerji M, Benoit-Lévy A, Bertin E, Brooks D, Rosell AC, Castander FJ, Costa LND, Covarrubias R, DePoy DL, Desai S, Diehl HT, Doel P, Eifler TF, Neto AF, Finley DA, Flaugher B, Fosalba P, Frieman J, Gerdes D, Gruen D, Gruendl RA, James D, Kuehn K, Kuropatkin N, Lahav O, Li TS, Maia MAG, Makler M, March M, Marshall JL, Martini P, Merritt KW, Miquel R, Nord B, Ogando R, Plazas AA, Romer AK, Roodman A, Sanchez E, Scarpine V, Schubnell M, Sevilla-Noarbe I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Walker AR. AUTOMATED TRANSIENT IDENTIFICATION IN THE DARK ENERGY SURVEY. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-6256/150/3/82] [Citation(s) in RCA: 94] [Impact Index Per Article: 10.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Drlica-Wagner A, Albert A, Bechtol K, Wood M, Strigari L, Sánchez-Conde M, Baldini L, Essig R, Cohen-Tanugi J, Anderson B, Bellazzini R, Bloom ED, Caputo R, Cecchi C, Charles E, Chiang J, Angelis AD, Funk S, Fusco P, Gargano F, Giglietto N, Giordano F, Guiriec S, Gustafsson M, Kuss M, Loparco F, Lubrano P, Mirabal N, Mizuno T, Morselli A, Ohsugi T, Orlando E, Persic M, Rainò S, Sehgal N, Spada F, Suson DJ, Zaharijas G, Zimmer S, Abbott T, Allam S, Balbinot E, Bauer AH, Benoit-Lévy A, Bernstein RA, Bernstein GM, Bertin E, Brooks D, Buckley-Geer E, Burke DL, Rosell AC, Castander FJ, Covarrubias R, D’Andrea CB, Costa LND, DePoy DL, Desai S, Diehl HT, Cunha CE, Eifler TF, Estrada J, Evrard AE, Neto AF, Fernandez E, Finley DA, Flaugher B, Frieman J, Gaztanaga E, Gerdes D, Gruen D, Gruendl RA, Gutierrez G, Honscheid K, Jain B, James D, Jeltema T, Kent S, Kron R, Kuehn K, Kuropatkin N, Lahav O, Li TS, Luque E, Maia MAG, Makler M, March M, Marshall J, Martini P, Merritt KW, Miller C, Miquel R, Mohr J, Neilsen E, Nord B, Ogando R, Peoples J, Petravick D, Pieres A, Plazas AA, Queiroz A, Romer AK, Roodman A, Rykoff ES, Sako M, Sanchez E, Santiago B, Scarpine V, Schubnell M, Sevilla I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Thomas D, Tucker D, Walker AR, Wechsler RH, Wester W, Williams P, Yanny B, Zuntz J. SEARCH FOR GAMMA-RAY EMISSION FROM DES DWARF SPHEROIDAL GALAXY CANDIDATES WITH
FERMI
-LAT DATA. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/2041-8205/809/1/l4] [Citation(s) in RCA: 119] [Impact Index Per Article: 13.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Chang C, Vikram V, Jain B, Bacon D, Amara A, Becker MR, Bernstein G, Bonnett C, Bridle S, Brout D, Busha M, Frieman J, Gaztanaga E, Hartley W, Jarvis M, Kacprzak T, Kovács A, Lahav O, Lin H, Melchior P, Peiris H, Rozo E, Rykoff E, Sánchez C, Sheldon E, Troxel MA, Wechsler R, Zuntz J, Abbott T, Abdalla FB, Allam S, Annis J, Bauer AH, Benoit-Lévy A, Brooks D, Buckley-Geer E, Burke DL, Capozzi D, Carnero Rosell A, Carrasco Kind M, Castander FJ, Crocce M, D'Andrea CB, Desai S, Diehl HT, Dietrich JP, Doel P, Eifler TF, Evrard AE, Fausti Neto A, Flaugher B, Fosalba P, Gruen D, Gruendl RA, Gutierrez G, Honscheid K, James D, Kent S, Kuehn K, Kuropatkin N, Maia MAG, March M, Martini P, Merritt KW, Miller CJ, Miquel R, Neilsen E, Nichol RC, Ogando R, Plazas AA, Romer AK, Roodman A, Sako M, Sanchez E, Sevilla I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Tarle G, Thaler J, Thomas D, Tucker D, Walker AR. Wide-Field Lensing Mass Maps from Dark Energy Survey Science Verification Data. Phys Rev Lett 2015; 115:051301. [PMID: 26274409 DOI: 10.1103/physrevlett.115.051301] [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: 05/07/2015] [Indexed: 06/04/2023]
Abstract
We present a mass map reconstructed from weak gravitational lensing shear measurements over 139 deg2 from the Dark Energy Survey science verification data. The mass map probes both luminous and dark matter, thus providing a tool for studying cosmology. We find good agreement between the mass map and the distribution of massive galaxy clusters identified using a red-sequence cluster finder. Potential candidates for superclusters and voids are identified using these maps. We measure the cross-correlation between the mass map and a magnitude-limited foreground galaxy sample and find a detection at the 6.8σ level with 20 arc min smoothing. These measurements are consistent with simulated galaxy catalogs based on N-body simulations from a cold dark matter model with a cosmological constant. This suggests low systematics uncertainties in the map. We summarize our key findings in this Letter; the detailed methodology and tests for systematics are presented in a companion paper.
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Affiliation(s)
- C Chang
- Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
| | - V Vikram
- Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - B Jain
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - D Bacon
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - A Amara
- Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
| | - M R Becker
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P. O. Box 2450, Stanford, California 94305, USA
| | - G Bernstein
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - C Bonnett
- Institut de Física d'Altes Energies, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Barcelona, Spain
| | - S Bridle
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, United Kingdom
| | - D Brout
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - M Busha
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P. O. Box 2450, Stanford, California 94305, USA
| | - J Frieman
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - E Gaztanaga
- Institut de Ciències de l'Espai, IEEC-CSIC, Campus UAB, Facultat de Ciències, Torre C5 par-2, 08193 Bellaterra, Barcelona, Spain
| | - W Hartley
- Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
| | - M Jarvis
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - T Kacprzak
- Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 16, CH-8093 Zurich, Switzerland
| | - A Kovács
- Institut de Física d'Altes Energies, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Barcelona, Spain
| | - O Lahav
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - H Lin
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - P Melchior
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - H Peiris
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - E Rozo
- Department of Physics, University of Arizona, 1118 East Fourth Street, Tucson, Arizona 85721, USA
| | - E Rykoff
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P. O. Box 2450, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - C Sánchez
- Institut de Física d'Altes Energies, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Barcelona, Spain
| | - E Sheldon
- Brookhaven National Laboratory, Building 510, Upton, New York 11973, USA
| | - M A Troxel
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, United Kingdom
| | - R Wechsler
- Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P. O. Box 2450, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - J Zuntz
- Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, United Kingdom
| | - T Abbott
- Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
| | - F B Abdalla
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - S Allam
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J Annis
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - A H Bauer
- Institut de Ciències de l'Espai, IEEC-CSIC, Campus UAB, Facultat de Ciències, Torre C5 par-2, 08193 Bellaterra, Barcelona, Spain
| | - A Benoit-Lévy
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - D Brooks
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - E Buckley-Geer
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - D L Burke
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P. O. Box 2450, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - D Capozzi
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - A Carnero Rosell
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Observatório Nacional, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - M Carrasco Kind
- Department of Physics, University of Illinois, 1110 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - F J Castander
- Institut de Ciències de l'Espai, IEEC-CSIC, Campus UAB, Facultat de Ciències, Torre C5 par-2, 08193 Bellaterra, Barcelona, Spain
| | - M Crocce
- Institut de Ciències de l'Espai, IEEC-CSIC, Campus UAB, Facultat de Ciències, Torre C5 par-2, 08193 Bellaterra, Barcelona, Spain
| | - C B D'Andrea
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - S Desai
- Department of Physics, Ludwig-Maximilians-Universitaet, Scheinerstrasse 1, 81679 Munich, Germany
| | - H T Diehl
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - J P Dietrich
- Department of Physics, Ludwig-Maximilians-Universitaet, Scheinerstrasse 1, 81679 Munich, Germany
- Excellence Cluster Universe, Boltzmannstrasse 2, 85748 Garching, Germany
| | - P Doel
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - T F Eifler
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - A E Evrard
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - A Fausti Neto
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - B Flaugher
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - P Fosalba
- Institut de Ciències de l'Espai, IEEC-CSIC, Campus UAB, Facultat de Ciències, Torre C5 par-2, 08193 Bellaterra, Barcelona, Spain
| | - D Gruen
- Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, 85748 Garching, Germany
- University Observatory Munich, Scheinerstrasse 1, 81679 Munich, Germany
| | - R A Gruendl
- Department of Physics, University of Illinois, 1110 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - G Gutierrez
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - K Honscheid
- Department of Physics, University of Illinois, 1110 West Green Street, Urbana, Illinois 61801, USA
- National Center for Supercomputing Applications, 1205 West Clark Street, Urbana, Illinois 61801, USA
| | - D James
- Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
| | - S Kent
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - K Kuehn
- Australian Astronomical Observatory, North Ryde, New South Wales 2113, Australia
| | - N Kuropatkin
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - M A G Maia
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Observatório Nacional, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - M March
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - P Martini
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - K W Merritt
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - C J Miller
- Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
- Department of Astronomy, University of Michigan, Ann Arbor, Michigan 48109, USA
| | - R Miquel
- Institut de Física d'Altes Energies, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Barcelona, Spain
- Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
| | - E Neilsen
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - R C Nichol
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
| | - R Ogando
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
- Observatório Nacional, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - A A Plazas
- Brookhaven National Laboratory, Building 510, Upton, New York 11973, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
| | - A K Romer
- Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, United Kingdom
| | - A Roodman
- Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, P. O. Box 2450, Stanford, California 94305, USA
- SLAC National Accelerator Laboratory, Menlo Park, California 94025, USA
| | - M Sako
- Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA
| | - E Sanchez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid 28040, Spain
| | - I Sevilla
- Department of Physics, University of Illinois, 1110 West Green Street, Urbana, Illinois 61801, USA
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid 28040, Spain
| | - R C Smith
- Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
| | - M Soares-Santos
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - F Sobreira
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
- Laboratório Interinstitucional de e-Astronomia-LIneA, Rua General Jos´e Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
| | - E Suchyta
- Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
| | - G Tarle
- Department of Physics, Ludwig-Maximilians-Universitaet, Scheinerstrasse 1, 81679 Munich, Germany
| | - J Thaler
- Department of Physics, University of Illinois, 1110 West Green Street, Urbana, Illinois 61801, USA
| | - D Thomas
- Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom
- SEPnet, South East Physics Network, Southampton SO17 1BJ, United Kingdom
| | - D Tucker
- Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510, USA
| | - A R Walker
- Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
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Simon JD, Drlica-Wagner A, Li TS, Nord B, Geha M, Bechtol K, Balbinot E, Buckley-Geer E, Lin H, Marshall J, Santiago B, Strigari L, Wang M, Wechsler RH, Yanny B, Abbott T, Bauer AH, Bernstein GM, Bertin E, Brooks D, Burke DL, Capozzi D, Rosell AC, Kind MC, D’Andrea CB, Costa LND, DePoy DL, Desai S, Diehl HT, Dodelson S, Cunha CE, Estrada J, Evrard AE, Neto AF, Fernandez E, Finley DA, Flaugher B, Frieman J, Gaztanaga E, Gerdes D, Gruen D, Gruendl RA, Honscheid K, James D, Kent S, Kuehn K, Kuropatkin N, Lahav O, Maia MAG, March M, Martini P, Miller CJ, Miquel R, Ogando R, Romer AK, Roodman A, Rykoff ES, Sako M, Sanchez E, Schubnell M, Sevilla I, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Tucker D, Vikram V, Walker AR, Wester W. STELLAR KINEMATICS AND METALLICITIES IN THE ULTRA-FAINT DWARF GALAXY RETICULUM II. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/808/1/95] [Citation(s) in RCA: 109] [Impact Index Per Article: 12.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Bechtol K, Drlica-Wagner A, Balbinot E, Pieres A, Simon JD, Yanny B, Santiago B, Wechsler RH, Frieman J, Walker AR, Williams P, Rozo E, Rykoff ES, Queiroz A, Luque E, Benoit-Lévy A, Tucker D, Sevilla I, Gruendl RA, Costa LND, Neto AF, Maia MAG, Abbott T, Allam S, Armstrong R, Bauer AH, Bernstein GM, Bernstein RA, Bertin E, Brooks D, Buckley-Geer E, Burke DL, Rosell AC, Castander FJ, Covarrubias R, D’Andrea CB, DePoy DL, Desai S, Diehl HT, Eifler TF, Estrada J, Evrard AE, Fernandez E, Finley DA, Flaugher B, Gaztanaga E, Gerdes D, Girardi L, Gladders M, Gruen D, Gutierrez G, Hao J, Honscheid K, Jain B, James D, Kent S, Kron R, Kuehn K, Kuropatkin N, Lahav O, Li TS, Lin H, Makler M, March M, Marshall J, Martini P, Merritt KW, Miller C, Miquel R, Mohr J, Neilsen E, Nichol R, Nord B, Ogando R, Peoples J, Petravick D, Plazas AA, Romer AK, Roodman A, Sako M, Sanchez E, Scarpine V, Schubnell M, Smith RC, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thaler J, Thomas D, Wester W, Zuntz J. EIGHT NEW MILKY WAY COMPANIONS DISCOVERED IN FIRST-YEAR DARK ENERGY SURVEY DATA. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/807/1/50] [Citation(s) in RCA: 401] [Impact Index Per Article: 44.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
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Merten J, Meneghetti M, Postman M, Umetsu K, Zitrin A, Medezinski E, Nonino M, Koekemoer A, Melchior P, Gruen D, Moustakas LA, Bartelmann M, Host O, Donahue M, Coe D, Molino A, Jouvel S, Monna A, Seitz S, Czakon N, Lemze D, Sayers J, Balestra I, Rosati P, Benítez N, Biviano A, Bouwens R, Bradley L, Broadhurst T, Carrasco M, Ford H, Grillo C, Infante L, Kelson D, Lahav O, Massey R, Moustakas J, Rasia E, Rhodes J, Vega J, Zheng W. CLASH: THE CONCENTRATION-MASS RELATION OF GALAXY CLUSTERS. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/806/1/4] [Citation(s) in RCA: 151] [Impact Index Per Article: 16.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Chang C, Busha MT, Wechsler RH, Refregier A, Amara A, Rykoff E, Becker MR, Bruderer C, Gamper L, Leistedt B, Peiris H, Abbott T, Abdalla FB, Balbinot E, Banerji M, Bernstein RA, Bertin E, Brooks D, Carnero A, Desai S, da Costa LN, Cunha CE, Eifler T, Evrard AE, Fausti Neto A, Gerdes D, Gruen D, James D, Kuehn K, Maia MAG, Makler M, Ogando R, Plazas A, Sanchez E, Santiago B, Schubnell M, Sevilla-Noarbe I, Smith C, Soares-Santos M, Suchyta E, Swanson MEC, Tarle G, Zuntz J. MODELING THE TRANSFER FUNCTION FOR THE DARK ENERGY SURVEY. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/801/2/73] [Citation(s) in RCA: 31] [Impact Index Per Article: 3.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Schneider R, Gruen D, Brause B. Diagnosis of infected joint prostheses. Semin Arthroplasty 1995; 6:167-75. [PMID: 10163522] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 02/11/2023]
Affiliation(s)
- R Schneider
- Department of Radiology and Medicine, Hospital for Special Surgery, New York, NY 10021, USA
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Zerah M, Ueshiba H, Wood E, Speiser PW, Crawford C, McDonald T, Pareira J, Gruen D, New MI. Prevalence of nonclassical steroid 21-hydroxylase deficiency based on a morning salivary 17-hydroxyprogesterone screening test: a small sample study. J Clin Endocrinol Metab 1990; 70:1662-7. [PMID: 2347899 DOI: 10.1210/jcem-70-6-1662] [Citation(s) in RCA: 45] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 12/31/2022]
Abstract
Early morning salivary 17 alpha-hydroxyprogesterone (17-OHP) determination differentiates patients with non-classical 21-hydroxylase deficiency (NC21OHD) from those who are not affected. Using this test, we have conducted a trial screening study for NC21OHD and have compared the study results with previously reported figures for the frequency of this disorder. Testing was performed on 258 subjects recruited from among the medical students and employees of the New York Hospital-Cornell Medical Center. In 2 of the 249 admissible subjects, the 0700-0900 h salivary 17-OHP level was within the range for NC21OHD patients (0.72-6.7 nmol/L; n = 8). These 2 individuals were subsequently confirmed to be affected by ACTH testing. Of the subjects with morning salivary 17-OHP levels below the cut-off point of 0.72 nmol/L, 29 were recalled for ACTH testing and were confirmed to be unaffected. Prevalence of NC21OHD in the test population was determined according to ethnic group. Our study gives a prevalence by screening of 1.14% among caucasians, which agrees with values of 0.81% and 1.06% obtained by different analytical methods. Further, both affected subjects were Ashkenazi Jews, and the prevalence of 3.23% among study members from this group concurs with increased rates of 3.64% and 4.97% already reported. On the basis of a small population sample, screening so far confirms the claim that NC21OHD is the most common autosomal recessive human disorder. Using values from ACTH-proven unaffected subjects (n = 47) and NC21OHD patients (n = 10), we establish preliminary normative data for morning salivary 17-OHP levels of 0.172 nmol/L for unaffected subjects (95% confidence interval, 0.05-0.54 nmol/L) and 1.76 nmol/L for NC21OHD-affected subjects (95% confidence interval, 0.42-7.32 nmol/L).
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Affiliation(s)
- M Zerah
- Department of Pediatrics, New York Hospital-Cornell Medical Center, New York 10021
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