A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES ...

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 $4.1 σ$ in c...

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Main Authors: 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., Rosell, A. Carnero, Kind, M. Carrasco, 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.
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Published: arXiv 2022
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Online Access:https://dx.doi.org/10.48550/arxiv.2207.11937
https://arxiv.org/abs/2207.11937
id ftdatacite:10.48550/arxiv.2207.11937
record_format openpolar
spelling ftdatacite:10.48550/arxiv.2207.11937 2023-07-23T04:21:48+02:00 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. Rosell, A. Carnero Kind, M. Carrasco 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. 2022 https://dx.doi.org/10.48550/arxiv.2207.11937 https://arxiv.org/abs/2207.11937 unknown arXiv https://dx.doi.org/10.1103/physrevd.107.042004 Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Text article-journal ScholarlyArticle Article 2022 ftdatacite https://doi.org/10.48550/arxiv.2207.1193710.1103/physrevd.107.042004 2023-07-03T21:13:14Z 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 $4.1 σ$ 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 $\barτ_e = (2.97 \pm 0.73) \times 10^{-3}$, while that inferred from the thermal SZ signal is $\barτ_e = (2.51 \pm 0.55^{\text{stat}} \pm 0.15^{\rm syst}) \times 10^{-3}$. The two measures agree at $0.6 σ$. We perform a suite of systematic checks to test the robustness of the analysis. ... Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
spellingShingle Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
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.
Rosell, A. Carnero
Kind, M. Carrasco
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.
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 Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
description 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 $4.1 σ$ 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 $\barτ_e = (2.97 \pm 0.73) \times 10^{-3}$, while that inferred from the thermal SZ signal is $\barτ_e = (2.51 \pm 0.55^{\text{stat}} \pm 0.15^{\rm syst}) \times 10^{-3}$. The two measures agree at $0.6 σ$. We perform a suite of systematic checks to test the robustness of the analysis. ...
format Text
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.
Rosell, A. Carnero
Kind, M. Carrasco
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.
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.
Rosell, A. Carnero
Kind, M. Carrasco
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.
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 arXiv
publishDate 2022
url https://dx.doi.org/10.48550/arxiv.2207.11937
https://arxiv.org/abs/2207.11937
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1103/physrevd.107.042004
op_rights Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
cc-by-4.0
op_doi https://doi.org/10.48550/arxiv.2207.1193710.1103/physrevd.107.042004
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