A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES
International audience We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The pairwise kSZ signal between pairs of clusters drawn from the DES Year-3 cluster catalog is d...
Published in: | Physical Review D |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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Online Access: | https://hal.science/hal-03759916 https://doi.org/10.1103/PhysRevD.107.042004 |
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ftccsdartic:oai:HAL:hal-03759916v1 2024-02-11T10:08:41+01:00 A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES Schiappucci, E. Bianchini, F. Aguena, M. Archipley, M. Balkenhol, L. Bleem, L.E. Chaubal, P. Crawford, T.M. Grandis, S. Omori, Y. Reichardt, C.L. Rozo, E. Rykoff, E.S. To, C. Abbott, T.M.C. Ade, P.A.R. Alves, O. Anderson, A.J. Andrade-Oliveira, F. Annis, J. Avva, J.S. Bacon, D. Benabed, K. Bender, A.N. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Bouchet, F.R. Brooks, D. Burke, D.L. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cecil, T.W. Chang, C.L. Chichura, P.M. Chou, T.-L. Costanzi, M. Cukierman, A. da Costa, L.N. Daley, C. de Haan, T. Desai, S. Dibert, K.R. Diehl, H.T. Dobbs, M.A. Doel, P. Doux, C. Dutcher, D. Everett, S. Everett, W. Feng, C. Ferguson, K.R. Ferrero, I. Ferté, A. Flaugher, B. Foster, A. Frieman, J. Galli, S. Gambrel, A.E. García-Bellido, J. Gardner, R.W. Gatti, M. Giannantonio, T. Goeckner-Wald, N. Gruen, D. Gualtieri, R. Guns, S. Gutierrez, G. Halverson, N.W. Hinton, S.R. Hivon, E. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hood, J.C. Huang, N. James, D.J. Knox, L. Korman, M. Kuehn, K. Kuo, C.-L. Lahav, O. Lee, A.T. Lidman, C. Lima, M. Lowitz, A.E. Lu, C. March, M. Mena-Fernández, J. Menanteau, F. Millea, M. Miquel, R. Mohr, J.J. Montgomery, J. Muir, J. Natoli, T. Noble, G.I. Novosad, V. Ogando, R.L.C. Padin, S. Pan, Z. Paz-Chinchón, F. Pereira, M.E.S. Pieres, A. Plazas Malagón, A.A. Prabhu, K. Prat, J. Quan, W. Rahlin, A. Raveri, M. Rodriguez-Monroy, M. Romer, A.K. Rouble, M. Ruhl, J.E. Sanchez, E. Scarpine, V. Schubnell, M. Smecher, G. Smith, M. Soares-Santos, M. Sobrin, J.A. Suchyta, E. Suzuki, A. Tarle, G. Thomas, D. Thompson, K.L. Thorne, B. Tucker, C. Umilta, C. Vieira, J.D. Vincenzi, M. Wang, G. Weaverdyck, N. Weller, J. Whitehorn, N. Wu, W.L.K. Yefremenko, V. Young, M.R. Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) SPT-3G DES 2023 https://hal.science/hal-03759916 https://doi.org/10.1103/PhysRevD.107.042004 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2207.11937 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.107.042004 hal-03759916 https://hal.science/hal-03759916 ARXIV: 2207.11937 doi:10.1103/PhysRevD.107.042004 INSPIRE: 2122660 Phys.Rev.D https://hal.science/hal-03759916 Phys.Rev.D, 2023, 107 (4), pp.042004. ⟨10.1103/PhysRevD.107.042004⟩ [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2023 ftccsdartic https://doi.org/10.1103/PhysRevD.107.042004 2024-01-14T00:08:20Z International audience We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The pairwise kSZ signal between pairs of clusters drawn from the DES Year-3 cluster catalog is detected at $4.1 \sigma$ in cosmic microwave background (CMB) temperature maps from two years of observations with the SPT-3G camera on the South Pole Telescope. After cuts, there are 24,580 clusters in the $\sim 1,400$ deg$^2$ of the southern sky observed by both experiments. We infer the mean optical depth of the cluster sample with two techniques. The optical depth inferred from the pairwise kSZ signal is $\bar{\tau}_e = (2.97 \pm 0.73) \times 10^{-3}$, while that inferred from the thermal SZ signal is $\bar{\tau}_e = (2.51 \pm 0.55) \times 10^{-3}$. The two measures agree at $0.6 \sigma$. We perform a suite of systematic checks to test the robustness of the analysis. Article in Journal/Newspaper South pole Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) South Pole Physical Review D 107 4 |
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Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
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ftccsdartic |
language |
English |
topic |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Schiappucci, E. Bianchini, F. Aguena, M. Archipley, M. Balkenhol, L. Bleem, L.E. Chaubal, P. Crawford, T.M. Grandis, S. Omori, Y. Reichardt, C.L. Rozo, E. Rykoff, E.S. To, C. Abbott, T.M.C. Ade, P.A.R. Alves, O. Anderson, A.J. Andrade-Oliveira, F. Annis, J. Avva, J.S. Bacon, D. Benabed, K. Bender, A.N. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Bouchet, F.R. Brooks, D. Burke, D.L. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cecil, T.W. Chang, C.L. Chichura, P.M. Chou, T.-L. Costanzi, M. Cukierman, A. da Costa, L.N. Daley, C. de Haan, T. Desai, S. Dibert, K.R. Diehl, H.T. Dobbs, M.A. Doel, P. Doux, C. Dutcher, D. Everett, S. Everett, W. Feng, C. Ferguson, K.R. Ferrero, I. Ferté, A. Flaugher, B. Foster, A. Frieman, J. Galli, S. Gambrel, A.E. García-Bellido, J. Gardner, R.W. Gatti, M. Giannantonio, T. Goeckner-Wald, N. Gruen, D. Gualtieri, R. Guns, S. Gutierrez, G. Halverson, N.W. Hinton, S.R. Hivon, E. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hood, J.C. Huang, N. James, D.J. Knox, L. Korman, M. Kuehn, K. Kuo, C.-L. Lahav, O. Lee, A.T. Lidman, C. Lima, M. Lowitz, A.E. Lu, C. March, M. Mena-Fernández, J. Menanteau, F. Millea, M. Miquel, R. Mohr, J.J. Montgomery, J. Muir, J. Natoli, T. Noble, G.I. Novosad, V. Ogando, R.L.C. Padin, S. Pan, Z. Paz-Chinchón, F. Pereira, M.E.S. Pieres, A. Plazas Malagón, A.A. Prabhu, K. Prat, J. Quan, W. Rahlin, A. Raveri, M. Rodriguez-Monroy, M. Romer, A.K. Rouble, M. Ruhl, J.E. Sanchez, E. Scarpine, V. Schubnell, M. Smecher, G. Smith, M. Soares-Santos, M. Sobrin, J.A. Suchyta, E. Suzuki, A. Tarle, G. Thomas, D. Thompson, K.L. Thorne, B. Tucker, C. Umilta, C. Vieira, J.D. Vincenzi, M. Wang, G. Weaverdyck, N. Weller, J. Whitehorn, N. Wu, W.L.K. Yefremenko, V. Young, M.R. A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES |
topic_facet |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The pairwise kSZ signal between pairs of clusters drawn from the DES Year-3 cluster catalog is detected at $4.1 \sigma$ in cosmic microwave background (CMB) temperature maps from two years of observations with the SPT-3G camera on the South Pole Telescope. After cuts, there are 24,580 clusters in the $\sim 1,400$ deg$^2$ of the southern sky observed by both experiments. We infer the mean optical depth of the cluster sample with two techniques. The optical depth inferred from the pairwise kSZ signal is $\bar{\tau}_e = (2.97 \pm 0.73) \times 10^{-3}$, while that inferred from the thermal SZ signal is $\bar{\tau}_e = (2.51 \pm 0.55) \times 10^{-3}$. The two measures agree at $0.6 \sigma$. We perform a suite of systematic checks to test the robustness of the analysis. |
author2 |
Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) SPT-3G DES |
format |
Article in Journal/Newspaper |
author |
Schiappucci, E. Bianchini, F. Aguena, M. Archipley, M. Balkenhol, L. Bleem, L.E. Chaubal, P. Crawford, T.M. Grandis, S. Omori, Y. Reichardt, C.L. Rozo, E. Rykoff, E.S. To, C. Abbott, T.M.C. Ade, P.A.R. Alves, O. Anderson, A.J. Andrade-Oliveira, F. Annis, J. Avva, J.S. Bacon, D. Benabed, K. Bender, A.N. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Bouchet, F.R. Brooks, D. Burke, D.L. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cecil, T.W. Chang, C.L. Chichura, P.M. Chou, T.-L. Costanzi, M. Cukierman, A. da Costa, L.N. Daley, C. de Haan, T. Desai, S. Dibert, K.R. Diehl, H.T. Dobbs, M.A. Doel, P. Doux, C. Dutcher, D. Everett, S. Everett, W. Feng, C. Ferguson, K.R. Ferrero, I. Ferté, A. Flaugher, B. Foster, A. Frieman, J. Galli, S. Gambrel, A.E. García-Bellido, J. Gardner, R.W. Gatti, M. Giannantonio, T. Goeckner-Wald, N. Gruen, D. Gualtieri, R. Guns, S. Gutierrez, G. Halverson, N.W. Hinton, S.R. Hivon, E. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hood, J.C. Huang, N. James, D.J. Knox, L. Korman, M. Kuehn, K. Kuo, C.-L. Lahav, O. Lee, A.T. Lidman, C. Lima, M. Lowitz, A.E. Lu, C. March, M. Mena-Fernández, J. Menanteau, F. Millea, M. Miquel, R. Mohr, J.J. Montgomery, J. Muir, J. Natoli, T. Noble, G.I. Novosad, V. Ogando, R.L.C. Padin, S. Pan, Z. Paz-Chinchón, F. Pereira, M.E.S. Pieres, A. Plazas Malagón, A.A. Prabhu, K. Prat, J. Quan, W. Rahlin, A. Raveri, M. Rodriguez-Monroy, M. Romer, A.K. Rouble, M. Ruhl, J.E. Sanchez, E. Scarpine, V. Schubnell, M. Smecher, G. Smith, M. Soares-Santos, M. Sobrin, J.A. Suchyta, E. Suzuki, A. Tarle, G. Thomas, D. Thompson, K.L. Thorne, B. Tucker, C. Umilta, C. Vieira, J.D. Vincenzi, M. Wang, G. Weaverdyck, N. Weller, J. Whitehorn, N. Wu, W.L.K. Yefremenko, V. Young, M.R. |
author_facet |
Schiappucci, E. Bianchini, F. Aguena, M. Archipley, M. Balkenhol, L. Bleem, L.E. Chaubal, P. Crawford, T.M. Grandis, S. Omori, Y. Reichardt, C.L. Rozo, E. Rykoff, E.S. To, C. Abbott, T.M.C. Ade, P.A.R. Alves, O. Anderson, A.J. Andrade-Oliveira, F. Annis, J. Avva, J.S. Bacon, D. Benabed, K. Bender, A.N. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Bouchet, F.R. Brooks, D. Burke, D.L. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cecil, T.W. Chang, C.L. Chichura, P.M. Chou, T.-L. Costanzi, M. Cukierman, A. da Costa, L.N. Daley, C. de Haan, T. Desai, S. Dibert, K.R. Diehl, H.T. Dobbs, M.A. Doel, P. Doux, C. Dutcher, D. Everett, S. Everett, W. Feng, C. Ferguson, K.R. Ferrero, I. Ferté, A. Flaugher, B. Foster, A. Frieman, J. Galli, S. Gambrel, A.E. García-Bellido, J. Gardner, R.W. Gatti, M. Giannantonio, T. Goeckner-Wald, N. Gruen, D. Gualtieri, R. Guns, S. Gutierrez, G. Halverson, N.W. Hinton, S.R. Hivon, E. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hood, J.C. Huang, N. James, D.J. Knox, L. Korman, M. Kuehn, K. Kuo, C.-L. Lahav, O. Lee, A.T. Lidman, C. Lima, M. Lowitz, A.E. Lu, C. March, M. Mena-Fernández, J. Menanteau, F. Millea, M. Miquel, R. Mohr, J.J. Montgomery, J. Muir, J. Natoli, T. Noble, G.I. Novosad, V. Ogando, R.L.C. Padin, S. Pan, Z. Paz-Chinchón, F. Pereira, M.E.S. Pieres, A. Plazas Malagón, A.A. Prabhu, K. Prat, J. Quan, W. Rahlin, A. Raveri, M. Rodriguez-Monroy, M. Romer, A.K. Rouble, M. Ruhl, J.E. Sanchez, E. Scarpine, V. Schubnell, M. Smecher, G. Smith, M. Soares-Santos, M. Sobrin, J.A. Suchyta, E. Suzuki, A. Tarle, G. Thomas, D. Thompson, K.L. Thorne, B. Tucker, C. Umilta, C. Vieira, J.D. Vincenzi, M. Wang, G. Weaverdyck, N. Weller, J. Whitehorn, N. Wu, W.L.K. Yefremenko, V. Young, M.R. |
author_sort |
Schiappucci, E. |
title |
A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES |
title_short |
A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES |
title_full |
A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES |
title_fullStr |
A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES |
title_full_unstemmed |
A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES |
title_sort |
measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic sunyaev-zel'dovich effect with spt-3g and des |
publisher |
HAL CCSD |
publishDate |
2023 |
url |
https://hal.science/hal-03759916 https://doi.org/10.1103/PhysRevD.107.042004 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Phys.Rev.D https://hal.science/hal-03759916 Phys.Rev.D, 2023, 107 (4), pp.042004. ⟨10.1103/PhysRevD.107.042004⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2207.11937 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.107.042004 hal-03759916 https://hal.science/hal-03759916 ARXIV: 2207.11937 doi:10.1103/PhysRevD.107.042004 INSPIRE: 2122660 |
op_doi |
https://doi.org/10.1103/PhysRevD.107.042004 |
container_title |
Physical Review D |
container_volume |
107 |
container_issue |
4 |
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1790608237791281152 |