COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY
We present cosmological parameter constraints obtained from galaxy clusters identified by their SunyaevZel'dovich effect signature in the 2500 square-degree South Pole Telescope Sunyaev Zel'dovich (SPT-SZ) survey. We consider the 377 cluster candidates identified at z > 0.25 with a dete...
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2016
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ndltd-arizona.edu-oai-arizona.openrepository.com-10150-6224522017-02-08T03:00:35Z 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. Univ Arizona, Steward Observ cosmology: observations galaxies: clusters: general We present cosmological parameter constraints obtained from galaxy clusters identified by their SunyaevZel'dovich effect signature in the 2500 square-degree South Pole Telescope Sunyaev Zel'dovich (SPT-SZ) 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 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 spatially flat Lambda CDM cosmology, we combine the cluster data with a prior on H-0 and find sigma(8)= 0.784. +/- 0.039 and Omega(m) = 0.289. +/- 0.042, with the parameter combination sigma(8) (Omega(m)/0.27)(0.3) = 0.797 +/- 0.031. These results are in good agreement with constraints from the cosmic microwave background (CMB) from SPT, WMAP, and Planck, as well as with constraints from other cluster data sets. We also consider several extensions to Lambda CDM, including models in which the equation of state of dark energy w, the species-summed neutrino mass, and/or the effective number of relativistic species (N-eff) are free parameters. When combined with constraints from the Planck CMB, H-0, baryon acoustic oscillation, and SNe, adding the SPT cluster data improves the w constraint by 14%, to w = -1.023 +/- 0.042. 2016-11-18 Article COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY 2016, 832 (1):95 The Astrophysical Journal 1538-4357 10.3847/0004-637X/832/1/95 http://hdl.handle.net/10150/622452 http://arizona.openrepository.com/arizona/handle/10150/622452 The Astrophysical Journal en http://stacks.iop.org/0004-637X/832/i=1/a=95?key=crossref.6a46975c233bedd2b937ec2e00c99d66 © 2016. The American Astronomical Society. All rights reserved. IOP PUBLISHING LTD |
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en |
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topic |
cosmology: observations galaxies: clusters: general |
spellingShingle |
cosmology: observations galaxies: clusters: general 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 |
description |
We present cosmological parameter constraints obtained from galaxy clusters identified by their SunyaevZel'dovich effect signature in the 2500 square-degree South Pole Telescope Sunyaev Zel'dovich (SPT-SZ) 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 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 spatially flat Lambda CDM cosmology, we combine the cluster data with a prior on H-0 and find sigma(8)= 0.784. +/- 0.039 and Omega(m) = 0.289. +/- 0.042, with the parameter combination sigma(8) (Omega(m)/0.27)(0.3) = 0.797 +/- 0.031. These results are in good agreement with constraints from the cosmic microwave background (CMB) from SPT, WMAP, and Planck, as well as with constraints from other cluster data sets. We also consider several extensions to Lambda CDM, including models in which the equation of state of dark energy w, the species-summed neutrino mass, and/or the effective number of relativistic species (N-eff) are free parameters. When combined with constraints from the Planck CMB, H-0, baryon acoustic oscillation, and SNe, adding the SPT cluster data improves the w constraint by 14%, to w = -1.023 +/- 0.042. |
author2 |
Univ Arizona, Steward Observ |
author_facet |
Univ Arizona, Steward Observ 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 |
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 |
publisher |
IOP PUBLISHING LTD |
publishDate |
2016 |
url |
http://hdl.handle.net/10150/622452 http://arizona.openrepository.com/arizona/handle/10150/622452 |
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