Validation of selection function, sample contamination and mass calibration in galaxy cluster samples
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 sele...
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OXFORD UNIV PRESS
2020
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ftucl:oai:eprints.ucl.ac.uk.OAI2:10117092 2023-12-24T10:24:54+01:00 Validation of selection function, sample contamination and mass calibration in galaxy cluster samples Grandis, S Klein, M Mohr, JJ Bocquet, S Paulus, M Abbott, TMC Aguena, M Allam, S Annis, J Benson, BA Bertin, E Bhargava, S Brooks, D Burke, DL Rosell, AC Kind, MC Carretero, J Capasso, R Costanzi, M da Costa, LN De Vicente, J Desai, S Dietrich, JP Doel, P Eifler, TF Evrard, AE Flaugher, B Fosalba, P Frieman, J Garcia-Bellido, J Gaztanaga, E Gerdes, DW Gruen, D Gruendl, RA Gschwend, J Gutierrez, G Hartley, WG Hinton, SR Hollowood, DL Honscheid, K James, DJ Jeltema, T Kuehn, K Kuropatkin, N Lima, M Maia, MAG Marshall, JL Melchior, P Menantcau, F Miquel, R Ogando, RLC Palmese, A Paz-Chinchon, E Plazas, AA Romer, AK Roodman, A Sanchez, E Saro, A Scarpine, V Schubnell, M Serrano, S Sheldon, E Smith, M Stark, AA Suchyta, E Swanson, MEC Tarle, G Thomas, D Tucker, DL Varga, TN Weller, J Wilkinson, R 2020-10 text https://discovery.ucl.ac.uk/id/eprint/10117092/1/staa2333.pdf https://discovery.ucl.ac.uk/id/eprint/10117092/ eng eng OXFORD UNIV PRESS https://discovery.ucl.ac.uk/id/eprint/10117092/1/staa2333.pdf https://discovery.ucl.ac.uk/id/eprint/10117092/ open Monthly Notices of the Royal Astronomical Society , 498 (1) pp. 771-798. (2020) methods: statistical galaxies: clusters: general large-scale structure of Universe X-rays: galaxies: clusters SOUTH-POLE TELESCOPE DARK ENERGY SURVEY WEAK-LENSING ANALYSIS X-RAY SCALING RELATIONS COSMOLOGICAL PARAMETERS CATALOG XMM CONSTRAINTS GIANTS Article 2020 ftucl 2023-11-27T13:07:39Z 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. Article in Journal/Newspaper South pole University College London: UCL Discovery South Pole |
institution |
Open Polar |
collection |
University College London: UCL Discovery |
op_collection_id |
ftucl |
language |
English |
topic |
methods: statistical galaxies: clusters: general large-scale structure of Universe X-rays: galaxies: clusters SOUTH-POLE TELESCOPE DARK ENERGY SURVEY WEAK-LENSING ANALYSIS X-RAY SCALING RELATIONS COSMOLOGICAL PARAMETERS CATALOG XMM CONSTRAINTS GIANTS |
spellingShingle |
methods: statistical galaxies: clusters: general large-scale structure of Universe X-rays: galaxies: clusters SOUTH-POLE TELESCOPE DARK ENERGY SURVEY WEAK-LENSING ANALYSIS X-RAY SCALING RELATIONS COSMOLOGICAL PARAMETERS CATALOG XMM CONSTRAINTS GIANTS Grandis, S Klein, M Mohr, JJ Bocquet, S Paulus, M Abbott, TMC Aguena, M Allam, S Annis, J Benson, BA Bertin, E Bhargava, S Brooks, D Burke, DL Rosell, AC Kind, MC Carretero, J Capasso, R Costanzi, M da Costa, LN De Vicente, J Desai, S Dietrich, JP Doel, P Eifler, TF Evrard, AE Flaugher, B Fosalba, P Frieman, J Garcia-Bellido, J Gaztanaga, E Gerdes, DW Gruen, D Gruendl, RA Gschwend, J Gutierrez, G Hartley, WG Hinton, SR Hollowood, DL Honscheid, K James, DJ Jeltema, T Kuehn, K Kuropatkin, N Lima, M Maia, MAG Marshall, JL Melchior, P Menantcau, F Miquel, R Ogando, RLC Palmese, A Paz-Chinchon, E Plazas, AA Romer, AK Roodman, A Sanchez, E Saro, A Scarpine, V Schubnell, M Serrano, S Sheldon, E Smith, M Stark, AA Suchyta, E Swanson, MEC Tarle, G Thomas, D Tucker, DL Varga, TN Weller, J Wilkinson, R Validation of selection function, sample contamination and mass calibration in galaxy cluster samples |
topic_facet |
methods: statistical galaxies: clusters: general large-scale structure of Universe X-rays: galaxies: clusters SOUTH-POLE TELESCOPE DARK ENERGY SURVEY WEAK-LENSING ANALYSIS X-RAY SCALING RELATIONS COSMOLOGICAL PARAMETERS CATALOG XMM CONSTRAINTS GIANTS |
description |
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. |
format |
Article in Journal/Newspaper |
author |
Grandis, S Klein, M Mohr, JJ Bocquet, S Paulus, M Abbott, TMC Aguena, M Allam, S Annis, J Benson, BA Bertin, E Bhargava, S Brooks, D Burke, DL Rosell, AC Kind, MC Carretero, J Capasso, R Costanzi, M da Costa, LN De Vicente, J Desai, S Dietrich, JP Doel, P Eifler, TF Evrard, AE Flaugher, B Fosalba, P Frieman, J Garcia-Bellido, J Gaztanaga, E Gerdes, DW Gruen, D Gruendl, RA Gschwend, J Gutierrez, G Hartley, WG Hinton, SR Hollowood, DL Honscheid, K James, DJ Jeltema, T Kuehn, K Kuropatkin, N Lima, M Maia, MAG Marshall, JL Melchior, P Menantcau, F Miquel, R Ogando, RLC Palmese, A Paz-Chinchon, E Plazas, AA Romer, AK Roodman, A Sanchez, E Saro, A Scarpine, V Schubnell, M Serrano, S Sheldon, E Smith, M Stark, AA Suchyta, E Swanson, MEC Tarle, G Thomas, D Tucker, DL Varga, TN Weller, J Wilkinson, R |
author_facet |
Grandis, S Klein, M Mohr, JJ Bocquet, S Paulus, M Abbott, TMC Aguena, M Allam, S Annis, J Benson, BA Bertin, E Bhargava, S Brooks, D Burke, DL Rosell, AC Kind, MC Carretero, J Capasso, R Costanzi, M da Costa, LN De Vicente, J Desai, S Dietrich, JP Doel, P Eifler, TF Evrard, AE Flaugher, B Fosalba, P Frieman, J Garcia-Bellido, J Gaztanaga, E Gerdes, DW Gruen, D Gruendl, RA Gschwend, J Gutierrez, G Hartley, WG Hinton, SR Hollowood, DL Honscheid, K James, DJ Jeltema, T Kuehn, K Kuropatkin, N Lima, M Maia, MAG Marshall, JL Melchior, P Menantcau, F Miquel, R Ogando, RLC Palmese, A Paz-Chinchon, E Plazas, AA Romer, AK Roodman, A Sanchez, E Saro, A Scarpine, V Schubnell, M Serrano, S Sheldon, E Smith, M Stark, AA Suchyta, E Swanson, MEC Tarle, G Thomas, D Tucker, DL Varga, TN Weller, J Wilkinson, R |
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 UNIV PRESS |
publishDate |
2020 |
url |
https://discovery.ucl.ac.uk/id/eprint/10117092/1/staa2333.pdf https://discovery.ucl.ac.uk/id/eprint/10117092/ |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Monthly Notices of the Royal Astronomical Society , 498 (1) pp. 771-798. (2020) |
op_relation |
https://discovery.ucl.ac.uk/id/eprint/10117092/1/staa2333.pdf https://discovery.ucl.ac.uk/id/eprint/10117092/ |
op_rights |
open |
_version_ |
1786200123421753344 |