Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements
We present a velocity dispersion-based mass calibration of the South Pole Telescope Sunyaev-Zel'dovich effect survey (SPT-SZ) galaxy cluster sample. Using a homogeneously selected sample of 100 cluster candidates from 720 deg2 of the survey along with 63 velocity dispersion ($σ_v$) and 16 X-ray...
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ftdatacite:10.48550/arxiv.1407.2942 2023-05-15T18:23:20+02:00 Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements Bocquet, S. Saro, A. Mohr, J. J. Aird, K. A. Ashby, M. L. N. Bautz, M. Bayliss, M. Bazin, G. Benson, B. A. Bleem, L. E. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H. M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. de Haan, T. Dietrich, J. P. Dobbs, M. A. Foley, R. J. Forman, W. R. Gangkofner, D. George, E. M. Gladders, M. D. Gonzalez, A. H. Halverson, N. W. Hennig, C. Hlavacek-Larrondo, J. Holder, G. P. Holzapfel, W. L. Hrubes, J. D. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Liu, J. Lueker, M. Luong-Van, D. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. Murray, S. S. Padin, S. Pryke, C. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Sayre, J. T. Schaffer, K. K. Shirokoff, E. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zahn, O. Zenteno, A. 2014 https://dx.doi.org/10.48550/arxiv.1407.2942 https://arxiv.org/abs/1407.2942 unknown arXiv https://dx.doi.org/10.1088/0004-637x/799/2/214 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences article-journal Article ScholarlyArticle Text 2014 ftdatacite https://doi.org/10.48550/arxiv.1407.2942 https://doi.org/10.1088/0004-637x/799/2/214 2022-04-01T12:52:41Z We present a velocity dispersion-based mass calibration of the South Pole Telescope Sunyaev-Zel'dovich effect survey (SPT-SZ) galaxy cluster sample. Using a homogeneously selected sample of 100 cluster candidates from 720 deg2 of the survey along with 63 velocity dispersion ($σ_v$) and 16 X-ray Yx measurements of sample clusters, we simultaneously calibrate the mass-observable relation and constrain cosmological parameters. The calibrations using $σ_v$ and Yx are consistent at the $0.6σ$ level, with the $σ_v$ calibration preferring ~16% higher masses. We use the full cluster dataset to measure $σ_8(Ω_ m/0.27)^{0.3}=0.809\pm0.036$. The SPT cluster abundance is lower than preferred by either the WMAP9 or Planck+WMAP9 polarization (WP) data, but assuming the sum of the neutrino masses is $\sum m_ν=0.06$ eV, we find the datasets to be consistent at the 1.0$σ$ level for WMAP9 and 1.5$σ$ for Planck+WP. Allowing for larger $\sum m_ν$ further reconciles the results. When we combine the cluster and Planck+WP datasets with BAO and SNIa, the preferred cluster masses are $1.9σ$ higher than the Yx calibration and $0.8σ$ higher than the $σ_v$ calibration. Given the scale of these shifts (~44% and ~23% in mass, respectively), we execute a goodness of fit test; it reveals no tension, indicating that the best-fit model provides an adequate description of the data. Using the multi-probe dataset, we measure $Ω_ m=0.299\pm0.009$ and $σ_8=0.829\pm0.011$. Within a $ν$CDM model we find $\sum m_ν= 0.148\pm0.081$ eV. We present a consistency test of the cosmic growth rate. Allowing both the growth index $γ$ and the dark energy equation of state parameter $w$ to vary, we find $γ=0.73\pm0.28$ and $w=-1.007\pm0.065$, demonstrating that the expansion and the growth histories are consistent with a LCDM model ($γ=0.55; \,w=-1$). : Accepted by ApJ (v2 is accepted version); 17 pages, 6 figures Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
spellingShingle |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Bocquet, S. Saro, A. Mohr, J. J. Aird, K. A. Ashby, M. L. N. Bautz, M. Bayliss, M. Bazin, G. Benson, B. A. Bleem, L. E. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H. M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. de Haan, T. Dietrich, J. P. Dobbs, M. A. Foley, R. J. Forman, W. R. Gangkofner, D. George, E. M. Gladders, M. D. Gonzalez, A. H. Halverson, N. W. Hennig, C. Hlavacek-Larrondo, J. Holder, G. P. Holzapfel, W. L. Hrubes, J. D. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Liu, J. Lueker, M. Luong-Van, D. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. Murray, S. S. Padin, S. Pryke, C. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Sayre, J. T. Schaffer, K. K. Shirokoff, E. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zahn, O. Zenteno, A. Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements |
topic_facet |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
We present a velocity dispersion-based mass calibration of the South Pole Telescope Sunyaev-Zel'dovich effect survey (SPT-SZ) galaxy cluster sample. Using a homogeneously selected sample of 100 cluster candidates from 720 deg2 of the survey along with 63 velocity dispersion ($σ_v$) and 16 X-ray Yx measurements of sample clusters, we simultaneously calibrate the mass-observable relation and constrain cosmological parameters. The calibrations using $σ_v$ and Yx are consistent at the $0.6σ$ level, with the $σ_v$ calibration preferring ~16% higher masses. We use the full cluster dataset to measure $σ_8(Ω_ m/0.27)^{0.3}=0.809\pm0.036$. The SPT cluster abundance is lower than preferred by either the WMAP9 or Planck+WMAP9 polarization (WP) data, but assuming the sum of the neutrino masses is $\sum m_ν=0.06$ eV, we find the datasets to be consistent at the 1.0$σ$ level for WMAP9 and 1.5$σ$ for Planck+WP. Allowing for larger $\sum m_ν$ further reconciles the results. When we combine the cluster and Planck+WP datasets with BAO and SNIa, the preferred cluster masses are $1.9σ$ higher than the Yx calibration and $0.8σ$ higher than the $σ_v$ calibration. Given the scale of these shifts (~44% and ~23% in mass, respectively), we execute a goodness of fit test; it reveals no tension, indicating that the best-fit model provides an adequate description of the data. Using the multi-probe dataset, we measure $Ω_ m=0.299\pm0.009$ and $σ_8=0.829\pm0.011$. Within a $ν$CDM model we find $\sum m_ν= 0.148\pm0.081$ eV. We present a consistency test of the cosmic growth rate. Allowing both the growth index $γ$ and the dark energy equation of state parameter $w$ to vary, we find $γ=0.73\pm0.28$ and $w=-1.007\pm0.065$, demonstrating that the expansion and the growth histories are consistent with a LCDM model ($γ=0.55; \,w=-1$). : Accepted by ApJ (v2 is accepted version); 17 pages, 6 figures |
format |
Text |
author |
Bocquet, S. Saro, A. Mohr, J. J. Aird, K. A. Ashby, M. L. N. Bautz, M. Bayliss, M. Bazin, G. Benson, B. A. Bleem, L. E. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H. M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. de Haan, T. Dietrich, J. P. Dobbs, M. A. Foley, R. J. Forman, W. R. Gangkofner, D. George, E. M. Gladders, M. D. Gonzalez, A. H. Halverson, N. W. Hennig, C. Hlavacek-Larrondo, J. Holder, G. P. Holzapfel, W. L. Hrubes, J. D. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Liu, J. Lueker, M. Luong-Van, D. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. Murray, S. S. Padin, S. Pryke, C. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Sayre, J. T. Schaffer, K. K. Shirokoff, E. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zahn, O. Zenteno, A. |
author_facet |
Bocquet, S. Saro, A. Mohr, J. J. Aird, K. A. Ashby, M. L. N. Bautz, M. Bayliss, M. Bazin, G. Benson, B. A. Bleem, L. E. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H. M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. de Haan, T. Dietrich, J. P. Dobbs, M. A. Foley, R. J. Forman, W. R. Gangkofner, D. George, E. M. Gladders, M. D. Gonzalez, A. H. Halverson, N. W. Hennig, C. Hlavacek-Larrondo, J. Holder, G. P. Holzapfel, W. L. Hrubes, J. D. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Liu, J. Lueker, M. Luong-Van, D. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. Murray, S. S. Padin, S. Pryke, C. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Sayre, J. T. Schaffer, K. K. Shirokoff, E. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zahn, O. Zenteno, A. |
author_sort |
Bocquet, S. |
title |
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements |
title_short |
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements |
title_full |
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements |
title_fullStr |
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements |
title_full_unstemmed |
Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $σ_v$ and X-ray $Y_\textrm{X}$ Measurements |
title_sort |
mass calibration and cosmological analysis of the spt-sz galaxy cluster sample using velocity dispersion $σ_v$ and x-ray $y_\textrm{x}$ measurements |
publisher |
arXiv |
publishDate |
2014 |
url |
https://dx.doi.org/10.48550/arxiv.1407.2942 https://arxiv.org/abs/1407.2942 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1088/0004-637x/799/2/214 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1407.2942 https://doi.org/10.1088/0004-637x/799/2/214 |
_version_ |
1766202903776722944 |