THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA
International audience We report the detection of the Sunyaev-Zel'dovich (SZ) effect of galaxy cluster XLSSU J021744.1-034536, using 30 GHz Combined Array for Research in Millimeter-wave Astronomy (CARMA) data. This cluster was discovered via its extended X-ray emission in the XMM-Newton Large...
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Online Access: | https://hal.science/hal-01442009 https://doi.org/10.1088/0004-637X/794/2/157 |
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ftunivaixmarseil:oai:HAL:hal-01442009v1 2024-04-28T08:38:52+00:00 THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA Mantz, A. B. Abdulla, Z. Carlstrom, J. E. Greer, C. H. Leitch, E. M. Marrone, D. P. Muchovej, S. Adami, C. Birkinshaw, M. Bremer, M. Clerc, N. Giles, P. Horellou, C. Maughan, B. Pacaud, F. Pierre, M. Willis, J. Laboratoire d'Astrophysique de Marseille (LAM) Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) AUTRES Max-Planck-Institut für Extraterrestrische Physik (MPE) Department of Earth and Space Sciences Göteborg Chalmers University of Technology Göteborg B. Maughan CEA/DCC/DRRV/SCD, Commissariat à l'Energie Atomique, Marcoule Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA) Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) 2014-10 https://hal.science/hal-01442009 https://doi.org/10.1088/0004-637X/794/2/157 en eng HAL CCSD American Astronomical Society info:eu-repo/semantics/altIdentifier/arxiv/1401.2087 info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/794/2/157 hal-01442009 https://hal.science/hal-01442009 ARXIV: 1401.2087 doi:10.1088/0004-637X/794/2/157 ISSN: 0004-637X EISSN: 1538-4357 The Astrophysical Journal https://hal.science/hal-01442009 The Astrophysical Journal, 2014, 794 (2), ⟨10.1088/0004-637X/794/2/157⟩ [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2014 ftunivaixmarseil https://doi.org/10.1088/0004-637X/794/2/157 2024-04-04T17:37:38Z International audience We report the detection of the Sunyaev-Zel'dovich (SZ) effect of galaxy cluster XLSSU J021744.1-034536, using 30 GHz Combined Array for Research in Millimeter-wave Astronomy (CARMA) data. This cluster was discovered via its extended X-ray emission in the XMM-Newton Large Scale Structure survey, the precursor to the XXL survey. It has a photometrically determined redshift z = 1.91(-0.21)(+0.19), making it among the most distant clusters known, and nominally the most distant for which the SZ effect has been measured. The spherically integrated Comptonization is Y-500 = (3.0 +/- 0.4) x 10(-12), a measurement that is relatively insensitive to assumptions regarding the size and redshift of the cluster, as well as the background cosmology. Using a variety of locally calibrated cluster scaling relations extrapolated to z similar to 2, we estimate a mass M-500 similar to (1-2) x 10(14) M-circle dot from the X-ray flux and SZ signal. The measured properties of this cluster are in good agreement with the extrapolation of an X-ray luminosity-SZ effect scaling relation calibrated from clusters discovered by the South Pole Telescope at higher masses and lower redshifts. The full XXL-CARMA sample will provide a more complete, multi-wavelength census of distant clusters in order to robustly extend the calibration of cluster scaling relations to these high redshifts. Article in Journal/Newspaper South pole Aix-Marseille Université: HAL The Astrophysical Journal 794 2 157 |
institution |
Open Polar |
collection |
Aix-Marseille Université: HAL |
op_collection_id |
ftunivaixmarseil |
language |
English |
topic |
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
spellingShingle |
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Mantz, A. B. Abdulla, Z. Carlstrom, J. E. Greer, C. H. Leitch, E. M. Marrone, D. P. Muchovej, S. Adami, C. Birkinshaw, M. Bremer, M. Clerc, N. Giles, P. Horellou, C. Maughan, B. Pacaud, F. Pierre, M. Willis, J. THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA |
topic_facet |
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
description |
International audience We report the detection of the Sunyaev-Zel'dovich (SZ) effect of galaxy cluster XLSSU J021744.1-034536, using 30 GHz Combined Array for Research in Millimeter-wave Astronomy (CARMA) data. This cluster was discovered via its extended X-ray emission in the XMM-Newton Large Scale Structure survey, the precursor to the XXL survey. It has a photometrically determined redshift z = 1.91(-0.21)(+0.19), making it among the most distant clusters known, and nominally the most distant for which the SZ effect has been measured. The spherically integrated Comptonization is Y-500 = (3.0 +/- 0.4) x 10(-12), a measurement that is relatively insensitive to assumptions regarding the size and redshift of the cluster, as well as the background cosmology. Using a variety of locally calibrated cluster scaling relations extrapolated to z similar to 2, we estimate a mass M-500 similar to (1-2) x 10(14) M-circle dot from the X-ray flux and SZ signal. The measured properties of this cluster are in good agreement with the extrapolation of an X-ray luminosity-SZ effect scaling relation calibrated from clusters discovered by the South Pole Telescope at higher masses and lower redshifts. The full XXL-CARMA sample will provide a more complete, multi-wavelength census of distant clusters in order to robustly extend the calibration of cluster scaling relations to these high redshifts. |
author2 |
Laboratoire d'Astrophysique de Marseille (LAM) Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS) AUTRES Max-Planck-Institut für Extraterrestrische Physik (MPE) Department of Earth and Space Sciences Göteborg Chalmers University of Technology Göteborg B. Maughan CEA/DCC/DRRV/SCD, Commissariat à l'Energie Atomique, Marcoule Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA) Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) |
format |
Article in Journal/Newspaper |
author |
Mantz, A. B. Abdulla, Z. Carlstrom, J. E. Greer, C. H. Leitch, E. M. Marrone, D. P. Muchovej, S. Adami, C. Birkinshaw, M. Bremer, M. Clerc, N. Giles, P. Horellou, C. Maughan, B. Pacaud, F. Pierre, M. Willis, J. |
author_facet |
Mantz, A. B. Abdulla, Z. Carlstrom, J. E. Greer, C. H. Leitch, E. M. Marrone, D. P. Muchovej, S. Adami, C. Birkinshaw, M. Bremer, M. Clerc, N. Giles, P. Horellou, C. Maughan, B. Pacaud, F. Pierre, M. Willis, J. |
author_sort |
Mantz, A. B. |
title |
THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA |
title_short |
THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA |
title_full |
THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA |
title_fullStr |
THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA |
title_full_unstemmed |
THE XXL SURVEY. V. DETECTION OF THE SUNYAEV-ZEL'DOVICH EFFECT OF THE REDSHIFT 1.9 GALAXY CLUSTER XLSSU J021744.1-034536 WITH CARMA |
title_sort |
xxl survey. v. detection of the sunyaev-zel'dovich effect of the redshift 1.9 galaxy cluster xlssu j021744.1-034536 with carma |
publisher |
HAL CCSD |
publishDate |
2014 |
url |
https://hal.science/hal-01442009 https://doi.org/10.1088/0004-637X/794/2/157 |
genre |
South pole |
genre_facet |
South pole |
op_source |
ISSN: 0004-637X EISSN: 1538-4357 The Astrophysical Journal https://hal.science/hal-01442009 The Astrophysical Journal, 2014, 794 (2), ⟨10.1088/0004-637X/794/2/157⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/1401.2087 info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/794/2/157 hal-01442009 https://hal.science/hal-01442009 ARXIV: 1401.2087 doi:10.1088/0004-637X/794/2/157 |
op_doi |
https://doi.org/10.1088/0004-637X/794/2/157 |
container_title |
The Astrophysical Journal |
container_volume |
794 |
container_issue |
2 |
container_start_page |
157 |
_version_ |
1797570119399899136 |