Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey
Here, we present cosmological constraints obtained from galaxy clusters identified by their Sunyaev-Zel'dovich effect signature in the 2500 square degree South Pole Telescope Sunyaev Zel'dovich survey. We consider the 377 cluster candidates identified at z>0.25 with a detection signific...
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Online Access: | http://www.osti.gov/servlets/purl/1349094 https://www.osti.gov/biblio/1349094 https://doi.org/10.3847/0004-637X/832/1/95 |
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ftosti:oai:osti.gov:1349094 2023-07-30T04:06:56+02:00 Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey Haan, T. de Benson, B. A. Bleem, L. E. Allen, S. W. Applegate, D. E. Ashby, M. L. N. Bautz, M. Bayliss, M. Bocquet, S. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H-M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. Dietrich, J. P. Dobbs, M. A. Doucouliagos, A. N. Foley, R. J. Forman, W. R. Garmire, G. P. George, E. M. Gladders, M. D. Gonzalez, A. H. Gupta, N. Halverson, N. W. Hlavacek-Larrondo, J. Hoekstra, H. Holder, G. P. Holzapfel, W. L. Hou, Z. Hrubes, J. D. Huang, N. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Linden, A. von der Luong-Van, D. Mantz, A. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. M. Mohr, J. J. Murray, S. S. Padin, S. Pryke, C. Rapetti, D. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Saro, A. Sayre, J. T. Schaffer, K. K. Schrabback, T. Shirokoff, E. Song, J. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. T. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zenteno, A. 2022-05-23 application/pdf http://www.osti.gov/servlets/purl/1349094 https://www.osti.gov/biblio/1349094 https://doi.org/10.3847/0004-637X/832/1/95 unknown http://www.osti.gov/servlets/purl/1349094 https://www.osti.gov/biblio/1349094 https://doi.org/10.3847/0004-637X/832/1/95 doi:10.3847/0004-637X/832/1/95 79 ASTRONOMY AND ASTROPHYSICS 2022 ftosti https://doi.org/10.3847/0004-637X/832/1/95 2023-07-11T09:17:48Z Here, we present cosmological constraints obtained from galaxy clusters identified by their Sunyaev-Zel'dovich effect signature in the 2500 square degree South Pole Telescope Sunyaev Zel'dovich survey. We consider the 377 cluster candidates identified at z>0.25 with a detection significance greater than five, corresponding to the 95% purity threshold for the survey. We compute constraints on cosmological models using the measured cluster abundance as a function of mass and redshift. We also include additional constraints from multi-wavelength observations, including Chandra X-ray data for 82 clusters and a weak lensing-based prior on the normalization of the mass-observable scaling relations. Assuming a LCDM cosmology, where the species-summed neutrino mass has the minimum allowed value (mnu = 0.06 eV) from neutrino oscillation experiments, we combine the cluster data with a prior on H0 and find σ 8 = 0.797±0.031 and Ω m = 0.289±0.042, with the parameter combination σ 8 (Ω m /0.27) 0.3 = 0.784±0.039. These results are in good agreement with constraints from the CMB from SPT, WMAP, and Planck, as well as with constraints from other cluster datasets. Adding mnu as a free parameter, we find mnu = 0.14±0.08 eV when combining the SPT cluster data with Planck CMB data and BAO data, consistent with the minimum allowed value. Finally, we consider a cosmology where mnu and N eff are fixed to the LCDM values, but the dark energy equation of state parameter w is free. Using the SPT cluster data in combination with an H 0 prior, we measure w = -1.28±0.31, a constraint consistent with the LCDM cosmological model and derived from the combination of growth of structure and geometry. When combined with primarily geometrical constraints from Planck CMB, H 0 , BAO and SNe, adding the SPT cluster data improves the w constraint from the geometrical data alone by 14%, to w = -1.023±0.042. Other/Unknown Material South pole SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) South Pole The Astrophysical Journal 832 1 95 |
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79 ASTRONOMY AND ASTROPHYSICS |
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79 ASTRONOMY AND ASTROPHYSICS Haan, T. de Benson, B. A. Bleem, L. E. Allen, S. W. Applegate, D. E. Ashby, M. L. N. Bautz, M. Bayliss, M. Bocquet, S. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H-M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. Dietrich, J. P. Dobbs, M. A. Doucouliagos, A. N. Foley, R. J. Forman, W. R. Garmire, G. P. George, E. M. Gladders, M. D. Gonzalez, A. H. Gupta, N. Halverson, N. W. Hlavacek-Larrondo, J. Hoekstra, H. Holder, G. P. Holzapfel, W. L. Hou, Z. Hrubes, J. D. Huang, N. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Linden, A. von der Luong-Van, D. Mantz, A. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. M. Mohr, J. J. Murray, S. S. Padin, S. Pryke, C. Rapetti, D. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Saro, A. Sayre, J. T. Schaffer, K. K. Schrabback, T. Shirokoff, E. Song, J. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. T. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zenteno, A. Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
topic_facet |
79 ASTRONOMY AND ASTROPHYSICS |
description |
Here, we present cosmological constraints obtained from galaxy clusters identified by their Sunyaev-Zel'dovich effect signature in the 2500 square degree South Pole Telescope Sunyaev Zel'dovich survey. We consider the 377 cluster candidates identified at z>0.25 with a detection significance greater than five, corresponding to the 95% purity threshold for the survey. We compute constraints on cosmological models using the measured cluster abundance as a function of mass and redshift. We also include additional constraints from multi-wavelength observations, including Chandra X-ray data for 82 clusters and a weak lensing-based prior on the normalization of the mass-observable scaling relations. Assuming a LCDM cosmology, where the species-summed neutrino mass has the minimum allowed value (mnu = 0.06 eV) from neutrino oscillation experiments, we combine the cluster data with a prior on H0 and find σ 8 = 0.797±0.031 and Ω m = 0.289±0.042, with the parameter combination σ 8 (Ω m /0.27) 0.3 = 0.784±0.039. These results are in good agreement with constraints from the CMB from SPT, WMAP, and Planck, as well as with constraints from other cluster datasets. Adding mnu as a free parameter, we find mnu = 0.14±0.08 eV when combining the SPT cluster data with Planck CMB data and BAO data, consistent with the minimum allowed value. Finally, we consider a cosmology where mnu and N eff are fixed to the LCDM values, but the dark energy equation of state parameter w is free. Using the SPT cluster data in combination with an H 0 prior, we measure w = -1.28±0.31, a constraint consistent with the LCDM cosmological model and derived from the combination of growth of structure and geometry. When combined with primarily geometrical constraints from Planck CMB, H 0 , BAO and SNe, adding the SPT cluster data improves the w constraint from the geometrical data alone by 14%, to w = -1.023±0.042. |
author |
Haan, T. de Benson, B. A. Bleem, L. E. Allen, S. W. Applegate, D. E. Ashby, M. L. N. Bautz, M. Bayliss, M. Bocquet, S. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H-M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. Dietrich, J. P. Dobbs, M. A. Doucouliagos, A. N. Foley, R. J. Forman, W. R. Garmire, G. P. George, E. M. Gladders, M. D. Gonzalez, A. H. Gupta, N. Halverson, N. W. Hlavacek-Larrondo, J. Hoekstra, H. Holder, G. P. Holzapfel, W. L. Hou, Z. Hrubes, J. D. Huang, N. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Linden, A. von der Luong-Van, D. Mantz, A. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. M. Mohr, J. J. Murray, S. S. Padin, S. Pryke, C. Rapetti, D. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Saro, A. Sayre, J. T. Schaffer, K. K. Schrabback, T. Shirokoff, E. Song, J. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. T. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zenteno, A. |
author_facet |
Haan, T. de Benson, B. A. Bleem, L. E. Allen, S. W. Applegate, D. E. Ashby, M. L. N. Bautz, M. Bayliss, M. Bocquet, S. Brodwin, M. Carlstrom, J. E. Chang, C. L. Chiu, I. Cho, H-M. Clocchiatti, A. Crawford, T. M. Crites, A. T. Desai, S. Dietrich, J. P. Dobbs, M. A. Doucouliagos, A. N. Foley, R. J. Forman, W. R. Garmire, G. P. George, E. M. Gladders, M. D. Gonzalez, A. H. Gupta, N. Halverson, N. W. Hlavacek-Larrondo, J. Hoekstra, H. Holder, G. P. Holzapfel, W. L. Hou, Z. Hrubes, J. D. Huang, N. Jones, C. Keisler, R. Knox, L. Lee, A. T. Leitch, E. M. Linden, A. von der Luong-Van, D. Mantz, A. Marrone, D. P. McDonald, M. McMahon, J. J. Meyer, S. S. Mocanu, L. M. Mohr, J. J. Murray, S. S. Padin, S. Pryke, C. Rapetti, D. Reichardt, C. L. Rest, A. Ruel, J. Ruhl, J. E. Saliwanchik, B. R. Saro, A. Sayre, J. T. Schaffer, K. K. Schrabback, T. Shirokoff, E. Song, J. Spieler, H. G. Stalder, B. Stanford, S. A. Staniszewski, Z. Stark, A. A. Story, K. T. Stubbs, C. W. Vanderlinde, K. Vieira, J. D. Vikhlinin, A. Williamson, R. Zenteno, A. |
author_sort |
Haan, T. de |
title |
Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
title_short |
Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
title_full |
Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
title_fullStr |
Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
title_full_unstemmed |
Cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
title_sort |
cosmological constraints from galaxy clusters in the 2500 square-degree spt-sz survey |
publishDate |
2022 |
url |
http://www.osti.gov/servlets/purl/1349094 https://www.osti.gov/biblio/1349094 https://doi.org/10.3847/0004-637X/832/1/95 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
http://www.osti.gov/servlets/purl/1349094 https://www.osti.gov/biblio/1349094 https://doi.org/10.3847/0004-637X/832/1/95 doi:10.3847/0004-637X/832/1/95 |
op_doi |
https://doi.org/10.3847/0004-637X/832/1/95 |
container_title |
The Astrophysical Journal |
container_volume |
832 |
container_issue |
1 |
container_start_page |
95 |
_version_ |
1772819896849137664 |