Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
We describe a method for measuring the integrated Comptonization (Y_(SZ)) of clusters of galaxies from measurements of the Sunyaev-Zel'dovich (SZ) effect in multiple frequency bands and use this method to characterize a sample of galaxy clusters detected in the South Pole Telescope (SPT) data....
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Online Access: | https://doi.org/10.1088/0004-637X/799/2/137 |
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ftcaltechauth:oai:authors.library.caltech.edu:cz3ag-9qn24 2024-06-23T07:56:49+00:00 Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope Saliwanchik, B. R. Lueker, M. Padin, S. Shirokoff, E. Vieira, J. D. 2015-02-01 https://doi.org/10.1088/0004-637X/799/2/137 unknown American Astronomical Society http://arxiv.org/abs/1312.3015 https://doi.org/10.1088/0004-637X/799/2/137 oai:authors.library.caltech.edu:cz3ag-9qn24 eprintid:55607 resolverid:CaltechAUTHORS:20150306-132050855 info:eu-repo/semantics/openAccess Other Astrophysical Journal, 799(2), Art. No. 137, (2015-02-01) galaxies: clusters: general methods: data analysis X-rays: galaxies: clusters info:eu-repo/semantics/article 2015 ftcaltechauth https://doi.org/10.1088/0004-637X/799/2/137 2024-06-12T05:19:35Z We describe a method for measuring the integrated Comptonization (Y_(SZ)) of clusters of galaxies from measurements of the Sunyaev-Zel'dovich (SZ) effect in multiple frequency bands and use this method to characterize a sample of galaxy clusters detected in the South Pole Telescope (SPT) data. We use a Markov Chain Monte Carlo method to fit a β-model source profile and integrate Y_(SZ) within an angular aperture on the sky. In simulated observations of an SPT-like survey that include cosmic microwave background anisotropy, point sources, and atmospheric and instrumental noise at typical SPT-SZ survey levels, we show that we can accurately recover β-model parameters for inputted clusters. We measure Y_(SZ) for simulated semi-analytic clusters and find that Y_(SZ) is most accurately determined in an angular aperture comparable to the SPT beam size. We demonstrate the utility of this method to measure Y_(SZ) and to constrain mass scaling relations using X-ray mass estimates for a sample of 18 galaxy clusters from the SPT-SZ survey. Measuring Y_(SZ) within a 0.'75 radius aperture, we find an intrinsic log-normal scatter of 21% ± 11% in Y_(SZ) at a fixed mass. Measuring Y_(SZ) within a 0.3 Mpc projected radius (equivalent to 0.'75 at the survey median redshift z = 0.6), we find a scatter of 26% ± 9%. Prior to this study, the SPT observable found to have the lowest scatter with mass was cluster detection significance. We demonstrate, from both simulations and SPT observed clusters that Y_(SZ) measured within an aperture comparable to the SPT beam size is equivalent, in terms of scatter with cluster mass, to SPT cluster detection significance. © 2015 American Astronomical Society. Received 2013 December 10; accepted 2014 November 20; published 2015 January 22. The South Pole Telescope program is supported by the National Science Foundation through grant ANT-0638937. Partial support is also provided by the NSF Physics Frontier Center grant PHY-0114422 to the Kavli Institute of Cosmological Physics at the ... Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) Kavli ENVELOPE(7.837,7.837,62.581,62.581) South Pole The Astrophysical Journal 799 2 137 |
institution |
Open Polar |
collection |
Caltech Authors (California Institute of Technology) |
op_collection_id |
ftcaltechauth |
language |
unknown |
topic |
galaxies: clusters: general methods: data analysis X-rays: galaxies: clusters |
spellingShingle |
galaxies: clusters: general methods: data analysis X-rays: galaxies: clusters Saliwanchik, B. R. Lueker, M. Padin, S. Shirokoff, E. Vieira, J. D. Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope |
topic_facet |
galaxies: clusters: general methods: data analysis X-rays: galaxies: clusters |
description |
We describe a method for measuring the integrated Comptonization (Y_(SZ)) of clusters of galaxies from measurements of the Sunyaev-Zel'dovich (SZ) effect in multiple frequency bands and use this method to characterize a sample of galaxy clusters detected in the South Pole Telescope (SPT) data. We use a Markov Chain Monte Carlo method to fit a β-model source profile and integrate Y_(SZ) within an angular aperture on the sky. In simulated observations of an SPT-like survey that include cosmic microwave background anisotropy, point sources, and atmospheric and instrumental noise at typical SPT-SZ survey levels, we show that we can accurately recover β-model parameters for inputted clusters. We measure Y_(SZ) for simulated semi-analytic clusters and find that Y_(SZ) is most accurately determined in an angular aperture comparable to the SPT beam size. We demonstrate the utility of this method to measure Y_(SZ) and to constrain mass scaling relations using X-ray mass estimates for a sample of 18 galaxy clusters from the SPT-SZ survey. Measuring Y_(SZ) within a 0.'75 radius aperture, we find an intrinsic log-normal scatter of 21% ± 11% in Y_(SZ) at a fixed mass. Measuring Y_(SZ) within a 0.3 Mpc projected radius (equivalent to 0.'75 at the survey median redshift z = 0.6), we find a scatter of 26% ± 9%. Prior to this study, the SPT observable found to have the lowest scatter with mass was cluster detection significance. We demonstrate, from both simulations and SPT observed clusters that Y_(SZ) measured within an aperture comparable to the SPT beam size is equivalent, in terms of scatter with cluster mass, to SPT cluster detection significance. © 2015 American Astronomical Society. Received 2013 December 10; accepted 2014 November 20; published 2015 January 22. The South Pole Telescope program is supported by the National Science Foundation through grant ANT-0638937. Partial support is also provided by the NSF Physics Frontier Center grant PHY-0114422 to the Kavli Institute of Cosmological Physics at the ... |
format |
Article in Journal/Newspaper |
author |
Saliwanchik, B. R. Lueker, M. Padin, S. Shirokoff, E. Vieira, J. D. |
author_facet |
Saliwanchik, B. R. Lueker, M. Padin, S. Shirokoff, E. Vieira, J. D. |
author_sort |
Saliwanchik, B. R. |
title |
Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope |
title_short |
Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope |
title_full |
Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope |
title_fullStr |
Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope |
title_full_unstemmed |
Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope |
title_sort |
measurement of galaxy cluster integrated comptonization and mass scaling relations with the south pole telescope |
publisher |
American Astronomical Society |
publishDate |
2015 |
url |
https://doi.org/10.1088/0004-637X/799/2/137 |
long_lat |
ENVELOPE(7.837,7.837,62.581,62.581) |
geographic |
Kavli South Pole |
geographic_facet |
Kavli South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Astrophysical Journal, 799(2), Art. No. 137, (2015-02-01) |
op_relation |
http://arxiv.org/abs/1312.3015 https://doi.org/10.1088/0004-637X/799/2/137 oai:authors.library.caltech.edu:cz3ag-9qn24 eprintid:55607 resolverid:CaltechAUTHORS:20150306-132050855 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1088/0004-637X/799/2/137 |
container_title |
The Astrophysical Journal |
container_volume |
799 |
container_issue |
2 |
container_start_page |
137 |
_version_ |
1802650164624621568 |