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 via the pairwise kinematic Sunyaev-Zel'dovich (KSZ) effect. The pairwise KSZ signal between pairs of clusters drawn from the Dark Energy Survey Year-3 cluster catalog is detected at 4.1...
Published in: | Physical Review D |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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2023
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Online Access: | https://researchers.mq.edu.au/en/publications/92343d6e-f636-4fc4-a799-b7f17f385c82 https://doi.org/10.1103/PhysRevD.107.042004 http://www.scopus.com/inward/record.url?scp=85150193159&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/DP200101068 |
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Macquarie University Research Portal |
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ftmacquarieunicr |
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English |
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We infer the mean optical depth of a sample of optically selected galaxy clusters from the Dark Energy Survey via the pairwise kinematic Sunyaev-Zel'dovich (KSZ) effect. The pairwise KSZ signal between pairs of clusters drawn from the Dark Energy Survey Year-3 cluster catalog is detected at 4.1σ in cosmic microwave background 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 ∼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 τ¯e=(2.97±0.73)×10 -3 , while that inferred from the thermal SZ signal is τ¯e=(2.51±0.55 stat ±0.15 syst )×10 -3 . The two measures agree at 0.6σ. We perform a suite of systematic checks to test the robustness of the analysis. |
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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. |
spellingShingle |
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. Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and des |
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 |
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 |
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 |
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 |
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 |
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 |
publishDate |
2023 |
url |
https://researchers.mq.edu.au/en/publications/92343d6e-f636-4fc4-a799-b7f17f385c82 https://doi.org/10.1103/PhysRevD.107.042004 http://www.scopus.com/inward/record.url?scp=85150193159&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/DP200101068 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
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 , Whi |
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https://doi.org/10.1103/PhysRevD.107.042004 |
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Physical Review D |
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107 |
container_issue |
4 |
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spelling |
ftmacquarieunicr:oai:https://researchers.mq.edu.au:publications/92343d6e-f636-4fc4-a799-b7f17f385c82 2024-10-13T14:10:50+00:00 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. 2023-02-15 https://researchers.mq.edu.au/en/publications/92343d6e-f636-4fc4-a799-b7f17f385c82 https://doi.org/10.1103/PhysRevD.107.042004 http://www.scopus.com/inward/record.url?scp=85150193159&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/DP200101068 eng eng info:eu-repo/semantics/closedAccess 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 , Whi article 2023 ftmacquarieunicr https://doi.org/10.1103/PhysRevD.107.042004 2024-10-03T00:23:13Z We infer the mean optical depth of a sample of optically selected galaxy clusters from the Dark Energy Survey via the pairwise kinematic Sunyaev-Zel'dovich (KSZ) effect. The pairwise KSZ signal between pairs of clusters drawn from the Dark Energy Survey Year-3 cluster catalog is detected at 4.1σ in cosmic microwave background 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 ∼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 τ¯e=(2.97±0.73)×10 -3 , while that inferred from the thermal SZ signal is τ¯e=(2.51±0.55 stat ±0.15 syst )×10 -3 . The two measures agree at 0.6σ. We perform a suite of systematic checks to test the robustness of the analysis. Article in Journal/Newspaper South pole Macquarie University Research Portal South Pole Physical Review D 107 4 |