Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters
We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg2 of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey science verification data. We identify 25 clusters between...
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ftinstnastrofisi:oai:openaccess.inaf.it:20.500.12386/27415 2023-05-15T18:23:00+02:00 Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters A. Saro S. Bocquet E. Rozo B. A. Benson J. Mohr E. S. Rykoff M. Soares-Santos L. Bleem S. Dodelson P. Melchior F. Sobreira V. Upadhyay J. Weller T. Abbott F. B. Abdalla S. Allam R. Armstrong M. Banerji A. H. Bauer M. Bayliss A. Benoit-Levy G. M. Bernstein E. Bertin M. Brodwin D. Brooks E. Buckley-Geer D. L. Burke J. E. Carlstrom R. Capasso D. Capozzi A. Carnero Rosell M. Carrasco Kind I. Chiu R. Covarrubias T. M. Crawford M. Crocce C. B. D'Andrea L. N. da Costa D. L. DePoy S. Desai T. de Haan H. T. Diehl J. P. Dietrich P. Doel C. E Cunha T. F. Eifler A. E. Evrard A. Fausti Neto E. Fernandez B. Flaugher 2015 https://hdl.handle.net/20.500.12386/27415 https://doi.org/10.1093/mnras/stv2141 http://arxiv.org/abs/1506.07814v1 https://academic.oup.com/mnras/article/454/3/2305/1201112 en eng MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 0035-8711 http://hdl.handle.net/20.500.12386/27415 doi:10.1093/mnras/stv2141 2-s2.0-85040254034 000368000400004 http://arxiv.org/abs/1506.07814v1 https://academic.oup.com/mnras/article/454/3/2305/1201112 2015MNRAS.454.2305S open Article 2015 ftinstnastrofisi https://doi.org/20.500.12386/27415 https://doi.org/10.1093/mnras/stv2141 2022-07-06T15:59:44Z We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg2 of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey science verification data. We identify 25 clusters between 0.1 ≲ z ≲ 0.8 in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness λ-mass relation with the following function <ln λ|M500> ∝ Bλln M500 + Cλln E(z) and use SPT-SZ cluster masses and RM richnesses λ to constrain the parameters. We find B_λ = 1.14^{+0.21}_{-0.18} and C_λ =0.73^{+0.77}_{-0.75}. The associated scatter in mass at fixed richness is σ _{ln M|λ } = 0.18^{+0.08}_{-0.05} at a characteristic richness λ = 70. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ-selected clusters with RM counterparts is consistent with expectations and that the fraction of RM-selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a subdominant population characterized by larger offsets. We also cross-match the RM catalogue with SPT-SZ candidates below the official catalogue threshold significance ξ = 4.5, using the RM catalogue to provide optical confirmation and redshifts for 15 additional clusters with ξ ∈ [4, 4.5]. Article in Journal/Newspaper South pole OA@INAF (Istituto Nazionale di Astrofisica) South Pole |
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OA@INAF (Istituto Nazionale di Astrofisica) |
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ftinstnastrofisi |
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English |
description |
We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg2 of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey science verification data. We identify 25 clusters between 0.1 ≲ z ≲ 0.8 in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness λ-mass relation with the following function <ln λ|M500> ∝ Bλln M500 + Cλln E(z) and use SPT-SZ cluster masses and RM richnesses λ to constrain the parameters. We find B_λ = 1.14^{+0.21}_{-0.18} and C_λ =0.73^{+0.77}_{-0.75}. The associated scatter in mass at fixed richness is σ _{ln M|λ } = 0.18^{+0.08}_{-0.05} at a characteristic richness λ = 70. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ-selected clusters with RM counterparts is consistent with expectations and that the fraction of RM-selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a subdominant population characterized by larger offsets. We also cross-match the RM catalogue with SPT-SZ candidates below the official catalogue threshold significance ξ = 4.5, using the RM catalogue to provide optical confirmation and redshifts for 15 additional clusters with ξ ∈ [4, 4.5]. |
format |
Article in Journal/Newspaper |
author |
A. Saro S. Bocquet E. Rozo B. A. Benson J. Mohr E. S. Rykoff M. Soares-Santos L. Bleem S. Dodelson P. Melchior F. Sobreira V. Upadhyay J. Weller T. Abbott F. B. Abdalla S. Allam R. Armstrong M. Banerji A. H. Bauer M. Bayliss A. Benoit-Levy G. M. Bernstein E. Bertin M. Brodwin D. Brooks E. Buckley-Geer D. L. Burke J. E. Carlstrom R. Capasso D. Capozzi A. Carnero Rosell M. Carrasco Kind I. Chiu R. Covarrubias T. M. Crawford M. Crocce C. B. D'Andrea L. N. da Costa D. L. DePoy S. Desai T. de Haan H. T. Diehl J. P. Dietrich P. Doel C. E Cunha T. F. Eifler A. E. Evrard A. Fausti Neto E. Fernandez B. Flaugher |
spellingShingle |
A. Saro S. Bocquet E. Rozo B. A. Benson J. Mohr E. S. Rykoff M. Soares-Santos L. Bleem S. Dodelson P. Melchior F. Sobreira V. Upadhyay J. Weller T. Abbott F. B. Abdalla S. Allam R. Armstrong M. Banerji A. H. Bauer M. Bayliss A. Benoit-Levy G. M. Bernstein E. Bertin M. Brodwin D. Brooks E. Buckley-Geer D. L. Burke J. E. Carlstrom R. Capasso D. Capozzi A. Carnero Rosell M. Carrasco Kind I. Chiu R. Covarrubias T. M. Crawford M. Crocce C. B. D'Andrea L. N. da Costa D. L. DePoy S. Desai T. de Haan H. T. Diehl J. P. Dietrich P. Doel C. E Cunha T. F. Eifler A. E. Evrard A. Fausti Neto E. Fernandez B. Flaugher Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters |
author_facet |
A. Saro S. Bocquet E. Rozo B. A. Benson J. Mohr E. S. Rykoff M. Soares-Santos L. Bleem S. Dodelson P. Melchior F. Sobreira V. Upadhyay J. Weller T. Abbott F. B. Abdalla S. Allam R. Armstrong M. Banerji A. H. Bauer M. Bayliss A. Benoit-Levy G. M. Bernstein E. Bertin M. Brodwin D. Brooks E. Buckley-Geer D. L. Burke J. E. Carlstrom R. Capasso D. Capozzi A. Carnero Rosell M. Carrasco Kind I. Chiu R. Covarrubias T. M. Crawford M. Crocce C. B. D'Andrea L. N. da Costa D. L. DePoy S. Desai T. de Haan H. T. Diehl J. P. Dietrich P. Doel C. E Cunha T. F. Eifler A. E. Evrard A. Fausti Neto E. Fernandez B. Flaugher |
author_sort |
A. Saro |
title |
Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters |
title_short |
Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters |
title_full |
Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters |
title_fullStr |
Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters |
title_full_unstemmed |
Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters |
title_sort |
constraints on the richness-mass relation and the optical-sze positional offset distribution for sze-selected clusters |
publishDate |
2015 |
url |
https://hdl.handle.net/20.500.12386/27415 https://doi.org/10.1093/mnras/stv2141 http://arxiv.org/abs/1506.07814v1 https://academic.oup.com/mnras/article/454/3/2305/1201112 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 0035-8711 http://hdl.handle.net/20.500.12386/27415 doi:10.1093/mnras/stv2141 2-s2.0-85040254034 000368000400004 http://arxiv.org/abs/1506.07814v1 https://academic.oup.com/mnras/article/454/3/2305/1201112 2015MNRAS.454.2305S |
op_rights |
open |
op_doi |
https://doi.org/20.500.12386/27415 https://doi.org/10.1093/mnras/stv2141 |
_version_ |
1766202424793497600 |