Validation of selection function, sample contamination and mass calibration in galaxy cluster samples
DES Collaboration: et al. We construct and validate the selection function of the MARD-Y3 galaxy cluster sample. This sample was selected through optical follow-up of the 2nd ROSAT faint source catalogue with Dark Energy Survey year 3 data. The selection function is modelled by combining an empirica...
Published in: | Monthly Notices of the Royal Astronomical Society |
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Oxford University Press
2020
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Online Access: | http://hdl.handle.net/10261/237566 https://doi.org/10.1093/mnras/staa2333 https://doi.org/10.13039/501100000781 https://doi.org/10.13039/501100000780 https://doi.org/10.13039/100000001 https://doi.org/10.13039/501100003329 https://doi.org/10.13039/501100002809 |
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Methods: statistical Galaxies: clusters: general X-rays: galaxies: clusters Large-scale structure of universe |
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Methods: statistical Galaxies: clusters: general X-rays: galaxies: clusters Large-scale structure of universe Grandis, S. Fosalba, Pablo García-Bellido, Juan Gaztañaga, Enrique Serrano, S. Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
topic_facet |
Methods: statistical Galaxies: clusters: general X-rays: galaxies: clusters Large-scale structure of universe |
description |
DES Collaboration: et al. We construct and validate the selection function of the MARD-Y3 galaxy cluster sample. This sample was selected through optical follow-up of the 2nd ROSAT faint source catalogue with Dark Energy Survey year 3 data. The selection function is modelled by combining an empirically constructed X-ray selection function with an incompleteness model for the optical follow-up. We validate the joint selection function by testing the consistency of the constraints on the X-ray flux–mass and richness–mass scaling relation parameters derived from different sources of mass information: (1) cross-calibration using South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) clusters, (2) calibration using number counts in X-ray, in optical and in both X-ray and optical while marginalizing over cosmological parameters, and (3) other published analyses. We find that the constraints on the scaling relation from the number counts and SPT-SZ cross-calibration agree, indicating that our modelling of the selection function is adequate. Furthermore, we apply a largely cosmology independent method to validate selection functions via the computation of the probability of finding each cluster in the SPT-SZ sample in the MARD-Y3 sample and vice versa. This test reveals no clear evidence for MARD-Y3 contamination, SPT-SZ incompleteness or outlier fraction. Finally, we discuss the prospects of the techniques presented here to limit systematic selection effects in future cluster cosmological studies. The DES data management system is supported by the National Science Foundation under grant numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015- 71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European ... |
author2 |
National Science Foundation (US) Ministerio de Economía y Competitividad (España) European Commission Generalitat de Catalunya European Research Council |
format |
Article in Journal/Newspaper |
author |
Grandis, S. Fosalba, Pablo García-Bellido, Juan Gaztañaga, Enrique Serrano, S. |
author_facet |
Grandis, S. Fosalba, Pablo García-Bellido, Juan Gaztañaga, Enrique Serrano, S. |
author_sort |
Grandis, S. |
title |
Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
title_short |
Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
title_full |
Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
title_fullStr |
Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
title_full_unstemmed |
Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
title_sort |
validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
publisher |
Oxford University Press |
publishDate |
2020 |
url |
http://hdl.handle.net/10261/237566 https://doi.org/10.1093/mnras/staa2333 https://doi.org/10.13039/501100000781 https://doi.org/10.13039/501100000780 https://doi.org/10.13039/100000001 https://doi.org/10.13039/501100003329 https://doi.org/10.13039/501100002809 |
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South Pole |
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South Pole |
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South pole |
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South pole |
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https://doi.org/10.1093/mnras/staa233310.13039/50110000078110.13039/50110000078010.13039/10000000110.13039/50110000332910.13039/501100002809 |
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Monthly Notices of the Royal Astronomical Society |
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ftcsic:oai:digital.csic.es:10261/237566 2024-02-11T10:08:43+01:00 Validation of selection function, sample contamination and mass calibration in galaxy cluster samples Grandis, S. Fosalba, Pablo García-Bellido, Juan Gaztañaga, Enrique Serrano, S. National Science Foundation (US) Ministerio de Economía y Competitividad (España) European Commission Generalitat de Catalunya European Research Council 2020 http://hdl.handle.net/10261/237566 https://doi.org/10.1093/mnras/staa2333 https://doi.org/10.13039/501100000781 https://doi.org/10.13039/501100000780 https://doi.org/10.13039/100000001 https://doi.org/10.13039/501100003329 https://doi.org/10.13039/501100002809 en eng Oxford University Press #PLACEHOLDER_PARENT_METADATA_VALUE# info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2015-71825 info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2015-66861 info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FPA2015-68048 info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/SEV-2016-0588 info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/SEV2016-0597 info:eu-repo/grantAgreement/EC/FP7/240672 info:eu-repo/grantAgreement/EC/FP7/291329 info:eu-repo/grantAgreement/EC/FP7/306478 Publisher's version https://doi.org/10.1093/mnras/staa2333 Sí Monthly Notices of the Royal Astronomical Society 498(1): 771–798 (2020) http://hdl.handle.net/10261/237566 doi:10.1093/mnras/staa2333 1365-2966 http://dx.doi.org/10.13039/501100000781 http://dx.doi.org/10.13039/501100000780 http://dx.doi.org/10.13039/100000001 http://dx.doi.org/10.13039/501100003329 http://dx.doi.org/10.13039/501100002809 open Methods: statistical Galaxies: clusters: general X-rays: galaxies: clusters Large-scale structure of universe artículo http://purl.org/coar/resource_type/c_6501 2020 ftcsic https://doi.org/10.1093/mnras/staa233310.13039/50110000078110.13039/50110000078010.13039/10000000110.13039/50110000332910.13039/501100002809 2024-01-16T11:06:57Z DES Collaboration: et al. We construct and validate the selection function of the MARD-Y3 galaxy cluster sample. This sample was selected through optical follow-up of the 2nd ROSAT faint source catalogue with Dark Energy Survey year 3 data. The selection function is modelled by combining an empirically constructed X-ray selection function with an incompleteness model for the optical follow-up. We validate the joint selection function by testing the consistency of the constraints on the X-ray flux–mass and richness–mass scaling relation parameters derived from different sources of mass information: (1) cross-calibration using South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) clusters, (2) calibration using number counts in X-ray, in optical and in both X-ray and optical while marginalizing over cosmological parameters, and (3) other published analyses. We find that the constraints on the scaling relation from the number counts and SPT-SZ cross-calibration agree, indicating that our modelling of the selection function is adequate. Furthermore, we apply a largely cosmology independent method to validate selection functions via the computation of the probability of finding each cluster in the SPT-SZ sample in the MARD-Y3 sample and vice versa. This test reveals no clear evidence for MARD-Y3 contamination, SPT-SZ incompleteness or outlier fraction. Finally, we discuss the prospects of the techniques presented here to limit systematic selection effects in future cluster cosmological studies. The DES data management system is supported by the National Science Foundation under grant numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015- 71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European ... Article in Journal/Newspaper South pole Digital.CSIC (Spanish National Research Council) South Pole Monthly Notices of the Royal Astronomical Society 498 1 771 798 |