SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets
International audience We present a Bayesian population modeling method to analyze the abundance of galaxy clusters identified by the South Pole Telescope (SPT) with a simultaneous mass calibration using weak gravitational lensing data from the Dark Energy Survey (DES) and the Hubble Space Telescope...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Other Authors: | , , , , , , , , , , , |
Format: | Report |
Language: | English |
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HAL CCSD
2023
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Subjects: | |
Online Access: | https://hal.science/hal-04266477 |
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ftunigrenoble:oai:HAL:hal-04266477v1 |
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record_format |
openpolar |
institution |
Open Polar |
collection |
Université Grenoble Alpes: HAL |
op_collection_id |
ftunigrenoble |
language |
English |
topic |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Bocquet, S Grandis, S Bleem, L.E Klein, M Mohr, J.J Aguena, M Alarcon, A Allam, S Allen, S.W Alves, O Amon, A Ansarinejad, B Bacon, D Bayliss, M Bechtol, K Becker, M.R Benson, B.A Bernstein, G.M Brodwin, M Brooks, D Campos, A Canning, R.E.A Carlstrom, J.E Carnero Rosell, A Carrasco Kind, M Carretero, J Cawthon, R Chang, C Chen, R Choi, A Cordero, J Costanzi, M da Costa, L.N Pereira, M.E.S Davis, C Derose, J Desai, S de Haan, T de Vicente, J Diehl, H.T Dodelson, S Doel, P Doux, C Drlica-Wagner, A Eckert, K Elvin-Poole, J Everett, S Ferrero, I Ferté, A Flores, A.M Frieman, J García-Bellido, J Gatti, M Giannini, G Gladders, M.D Gruen, D Gruendl, R.A Harrison, I Hartley, W.G Herner, K Hinton, S.R Hollowood, D.L Holzapfel, W.L Honscheid, K Huang, N Huff, E.M James, D.J Jarvis, M Khullar, G Kim, K Kraft, R Kuehn, K Kuropatkin, N Kéruzoré, F Lee, S Leget, P.-F Maccrann, N Mahler, G Mantz, A Marshall, J.L Mccullough, J Mcdonald, M Mena-Fernández, J Miquel, R Myles, J Navarro-Alsina, A Ogando, R.L.C Palmese, A Pandey, S Pieres, A Plazas Malagón, A.A Prat, J Raveri, M Reichardt, C.L Roberson, J Rollins, R.P Romer, A.K Romero, C Roodman, A Ross, A.J Rykoff, E.S Salvati, L Sánchez, C Sanchez, E Sanchez Cid, D Saro, A Schrabback, T Schubnell, M Secco, L.F Sevilla-Noarbe, I Sharon, K Sheldon, E Shin, T Smith, M Somboonpanyakul, T Stalder, B Stark, A.A Strazzullo, V Suchyta, E Swanson, M.E.C Tarle, G To, C Troxel, M.A Tutusaus, I Varga, T.N von der Linden, A Weaverdyck, N Weller, J Wiseman, P Yanny, B Yin, B Young, M Zhang, Y Zuntz, J SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets |
topic_facet |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience We present a Bayesian population modeling method to analyze the abundance of galaxy clusters identified by the South Pole Telescope (SPT) with a simultaneous mass calibration using weak gravitational lensing data from the Dark Energy Survey (DES) and the Hubble Space Telescope (HST). We discuss and validate the modeling choices with a particular focus on a robust, weak-lensing-based mass calibration using DES data. For the DES Year 3 data, we report a systematic uncertainty in weak-lensing mass calibration that increases from 1% at $z=0.25$ to 10% at $z=0.95$, to which we add 2% in quadrature to account for uncertainties in the impact of baryonic effects. We implement an analysis pipeline that joins the cluster abundance likelihood with a multi-observable likelihood for the SZ, optical richness, and weak-lensing measurements for each individual cluster. We validate that our analysis pipeline can recover unbiased cosmological constraints by analyzing mocks that closely resemble the cluster sample extracted from the SPT-SZ, SPTpol~ECS, and SPTpol~500d surveys and the DES Year~3 and HST-39 weak-lensing datasets. This work represents a crucial prerequisite for the subsequent cosmological analysis of the real dataset. |
author2 |
Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ) Université Grenoble Alpes (UGA) Institut d'astrophysique spatiale (IAS) Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) Institut de recherche en astrophysique et planétologie (IRAP) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) DES SPT |
format |
Report |
author |
Bocquet, S Grandis, S Bleem, L.E Klein, M Mohr, J.J Aguena, M Alarcon, A Allam, S Allen, S.W Alves, O Amon, A Ansarinejad, B Bacon, D Bayliss, M Bechtol, K Becker, M.R Benson, B.A Bernstein, G.M Brodwin, M Brooks, D Campos, A Canning, R.E.A Carlstrom, J.E Carnero Rosell, A Carrasco Kind, M Carretero, J Cawthon, R Chang, C Chen, R Choi, A Cordero, J Costanzi, M da Costa, L.N Pereira, M.E.S Davis, C Derose, J Desai, S de Haan, T de Vicente, J Diehl, H.T Dodelson, S Doel, P Doux, C Drlica-Wagner, A Eckert, K Elvin-Poole, J Everett, S Ferrero, I Ferté, A Flores, A.M Frieman, J García-Bellido, J Gatti, M Giannini, G Gladders, M.D Gruen, D Gruendl, R.A Harrison, I Hartley, W.G Herner, K Hinton, S.R Hollowood, D.L Holzapfel, W.L Honscheid, K Huang, N Huff, E.M James, D.J Jarvis, M Khullar, G Kim, K Kraft, R Kuehn, K Kuropatkin, N Kéruzoré, F Lee, S Leget, P.-F Maccrann, N Mahler, G Mantz, A Marshall, J.L Mccullough, J Mcdonald, M Mena-Fernández, J Miquel, R Myles, J Navarro-Alsina, A Ogando, R.L.C Palmese, A Pandey, S Pieres, A Plazas Malagón, A.A Prat, J Raveri, M Reichardt, C.L Roberson, J Rollins, R.P Romer, A.K Romero, C Roodman, A Ross, A.J Rykoff, E.S Salvati, L Sánchez, C Sanchez, E Sanchez Cid, D Saro, A Schrabback, T Schubnell, M Secco, L.F Sevilla-Noarbe, I Sharon, K Sheldon, E Shin, T Smith, M Somboonpanyakul, T Stalder, B Stark, A.A Strazzullo, V Suchyta, E Swanson, M.E.C Tarle, G To, C Troxel, M.A Tutusaus, I Varga, T.N von der Linden, A Weaverdyck, N Weller, J Wiseman, P Yanny, B Yin, B Young, M Zhang, Y Zuntz, J |
author_facet |
Bocquet, S Grandis, S Bleem, L.E Klein, M Mohr, J.J Aguena, M Alarcon, A Allam, S Allen, S.W Alves, O Amon, A Ansarinejad, B Bacon, D Bayliss, M Bechtol, K Becker, M.R Benson, B.A Bernstein, G.M Brodwin, M Brooks, D Campos, A Canning, R.E.A Carlstrom, J.E Carnero Rosell, A Carrasco Kind, M Carretero, J Cawthon, R Chang, C Chen, R Choi, A Cordero, J Costanzi, M da Costa, L.N Pereira, M.E.S Davis, C Derose, J Desai, S de Haan, T de Vicente, J Diehl, H.T Dodelson, S Doel, P Doux, C Drlica-Wagner, A Eckert, K Elvin-Poole, J Everett, S Ferrero, I Ferté, A Flores, A.M Frieman, J García-Bellido, J Gatti, M Giannini, G Gladders, M.D Gruen, D Gruendl, R.A Harrison, I Hartley, W.G Herner, K Hinton, S.R Hollowood, D.L Holzapfel, W.L Honscheid, K Huang, N Huff, E.M James, D.J Jarvis, M Khullar, G Kim, K Kraft, R Kuehn, K Kuropatkin, N Kéruzoré, F Lee, S Leget, P.-F Maccrann, N Mahler, G Mantz, A Marshall, J.L Mccullough, J Mcdonald, M Mena-Fernández, J Miquel, R Myles, J Navarro-Alsina, A Ogando, R.L.C Palmese, A Pandey, S Pieres, A Plazas Malagón, A.A Prat, J Raveri, M Reichardt, C.L Roberson, J Rollins, R.P Romer, A.K Romero, C Roodman, A Ross, A.J Rykoff, E.S Salvati, L Sánchez, C Sanchez, E Sanchez Cid, D Saro, A Schrabback, T Schubnell, M Secco, L.F Sevilla-Noarbe, I Sharon, K Sheldon, E Shin, T Smith, M Somboonpanyakul, T Stalder, B Stark, A.A Strazzullo, V Suchyta, E Swanson, M.E.C Tarle, G To, C Troxel, M.A Tutusaus, I Varga, T.N von der Linden, A Weaverdyck, N Weller, J Wiseman, P Yanny, B Yin, B Young, M Zhang, Y Zuntz, J |
author_sort |
Bocquet, S |
title |
SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets |
title_short |
SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets |
title_full |
SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets |
title_fullStr |
SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets |
title_full_unstemmed |
SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets |
title_sort |
spt clusters with des and hst weak lensing. i. cluster lensing and bayesian population modeling of multi-wavelength cluster datasets |
publisher |
HAL CCSD |
publishDate |
2023 |
url |
https://hal.science/hal-04266477 |
long_lat |
ENVELOPE(158.317,158.317,-80.867,-80.867) |
geographic |
Hubble South Pole |
geographic_facet |
Hubble South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
https://hal.science/hal-04266477 2023 |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2310.12213 hal-04266477 https://hal.science/hal-04266477 ARXIV: 2310.12213 INSPIRE: 2712796 |
_version_ |
1809943229877977088 |
spelling |
ftunigrenoble:oai:HAL:hal-04266477v1 2024-09-09T20:09:06+00:00 SPT Clusters with DES and HST Weak Lensing. I. Cluster Lensing and Bayesian Population Modeling of Multi-Wavelength Cluster Datasets Bocquet, S Grandis, S Bleem, L.E Klein, M Mohr, J.J Aguena, M Alarcon, A Allam, S Allen, S.W Alves, O Amon, A Ansarinejad, B Bacon, D Bayliss, M Bechtol, K Becker, M.R Benson, B.A Bernstein, G.M Brodwin, M Brooks, D Campos, A Canning, R.E.A Carlstrom, J.E Carnero Rosell, A Carrasco Kind, M Carretero, J Cawthon, R Chang, C Chen, R Choi, A Cordero, J Costanzi, M da Costa, L.N Pereira, M.E.S Davis, C Derose, J Desai, S de Haan, T de Vicente, J Diehl, H.T Dodelson, S Doel, P Doux, C Drlica-Wagner, A Eckert, K Elvin-Poole, J Everett, S Ferrero, I Ferté, A Flores, A.M Frieman, J García-Bellido, J Gatti, M Giannini, G Gladders, M.D Gruen, D Gruendl, R.A Harrison, I Hartley, W.G Herner, K Hinton, S.R Hollowood, D.L Holzapfel, W.L Honscheid, K Huang, N Huff, E.M James, D.J Jarvis, M Khullar, G Kim, K Kraft, R Kuehn, K Kuropatkin, N Kéruzoré, F Lee, S Leget, P.-F Maccrann, N Mahler, G Mantz, A Marshall, J.L Mccullough, J Mcdonald, M Mena-Fernández, J Miquel, R Myles, J Navarro-Alsina, A Ogando, R.L.C Palmese, A Pandey, S Pieres, A Plazas Malagón, A.A Prat, J Raveri, M Reichardt, C.L Roberson, J Rollins, R.P Romer, A.K Romero, C Roodman, A Ross, A.J Rykoff, E.S Salvati, L Sánchez, C Sanchez, E Sanchez Cid, D Saro, A Schrabback, T Schubnell, M Secco, L.F Sevilla-Noarbe, I Sharon, K Sheldon, E Shin, T Smith, M Somboonpanyakul, T Stalder, B Stark, A.A Strazzullo, V Suchyta, E Swanson, M.E.C Tarle, G To, C Troxel, M.A Tutusaus, I Varga, T.N von der Linden, A Weaverdyck, N Weller, J Wiseman, P Yanny, B Yin, B Young, M Zhang, Y Zuntz, J Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ) Université Grenoble Alpes (UGA) Institut d'astrophysique spatiale (IAS) Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) Institut de recherche en astrophysique et planétologie (IRAP) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) DES SPT 2023-10-31 https://hal.science/hal-04266477 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2310.12213 hal-04266477 https://hal.science/hal-04266477 ARXIV: 2310.12213 INSPIRE: 2712796 https://hal.science/hal-04266477 2023 [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/preprint Preprints, Working Papers, . 2023 ftunigrenoble 2024-07-29T23:39:57Z International audience We present a Bayesian population modeling method to analyze the abundance of galaxy clusters identified by the South Pole Telescope (SPT) with a simultaneous mass calibration using weak gravitational lensing data from the Dark Energy Survey (DES) and the Hubble Space Telescope (HST). We discuss and validate the modeling choices with a particular focus on a robust, weak-lensing-based mass calibration using DES data. For the DES Year 3 data, we report a systematic uncertainty in weak-lensing mass calibration that increases from 1% at $z=0.25$ to 10% at $z=0.95$, to which we add 2% in quadrature to account for uncertainties in the impact of baryonic effects. We implement an analysis pipeline that joins the cluster abundance likelihood with a multi-observable likelihood for the SZ, optical richness, and weak-lensing measurements for each individual cluster. We validate that our analysis pipeline can recover unbiased cosmological constraints by analyzing mocks that closely resemble the cluster sample extracted from the SPT-SZ, SPTpol~ECS, and SPTpol~500d surveys and the DES Year~3 and HST-39 weak-lensing datasets. This work represents a crucial prerequisite for the subsequent cosmological analysis of the real dataset. Report South pole Université Grenoble Alpes: HAL Hubble ENVELOPE(158.317,158.317,-80.867,-80.867) South Pole |