Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
International audience We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-$y$-maps generated using data from the South Pole Telescope (SPT) and the {\it Planck} mission. We model this cross-correlation measurement together with...
Published in: | Monthly Notices of the Royal Astronomical Society |
---|---|
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2023
|
Subjects: | |
Online Access: | https://hal.science/hal-03826315 https://hal.science/hal-03826315/document https://hal.science/hal-03826315/file/stad1167.pdf https://doi.org/10.1093/mnras/stad1167 |
id |
ftinsu:oai:HAL:hal-03826315v1 |
---|---|
record_format |
openpolar |
institution |
Open Polar |
collection |
Institut national des sciences de l'Univers: HAL-INSU |
op_collection_id |
ftinsu |
language |
English |
topic |
galaxies: structure large-scale structure of Universe cosmology: observations [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
galaxies: structure large-scale structure of Universe cosmology: observations [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Omori, Y. Chang, C. Bleem, L.E. Crawford, T. Drlica-Wagner, A. Raghunathan, S. Zacharegkas, G. Abbott, T.M.C. Aguena, M. Alarcon, A. Allam, S. Alves, O. Amon, A. Avila, S. Baxter, E. Bechtol, K. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Brooks, D. Burke, D.L. Campos, A. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Chang, C.L. Chen, A. Choi, A. Chown, R. Costanzi, M. Crites, A.T. Crocce, M. da Costa, L.N. Pereira, M.E.S. de Haan, T. de Vicente, J. Derose, J. Desai, S. Diehl, H.T. Dobbs, M.A. Dodelson, S. Doel, P. Elvin-Poole, J. Everett, W. Everett, S. Ferrero, I. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gatti, M. George, E.M. Gerdes, D.W. Giannini, G. Gruen, D. Gruendl, R.A. Gschwend, J. Gutierrez, G. Halverson, N.W. Hinton, S.R. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hrubes, J.D. James, D.J. Knox, L. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, A.T. Luong-Van, D. Maccrann, N. Marshall, J.L. Mccullough, J. Mcmahon, J.J. Melchior, P. Mena-Fernández, J. Menanteau, F. Miquel, R. Mocanu, L. Mohr, J.J. Muir, J. Myles, J. Natoli, T. Padin, S. Palmese, A. Pandey, S. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A.A. Porredon, A. Pryke, C. Raveri, M. Reichardt, C.L. Rodriguez-Monroy, M. Ross, A.J. Ruhl, J.E. Rykoff, E. Sánchez, C. Sanchez, E. Scarpine, V. Schaffer, K.K. Sevilla-Noarbe, I. Sheldon, E. Shirokoff, E. Smith, M. Soares-Santos, M. Staniszewski, Z. Stark, A.A. Suchyta, E. Tarle, G. Thomas, D. Troxel, M.A. Tucker, D.L. Vieira, J.D. Vincenzi, M. Weaverdyck, N. Williamson, R. Yanny, B. Yin, B. Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck |
topic_facet |
galaxies: structure large-scale structure of Universe cosmology: observations [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-$y$-maps generated using data from the South Pole Telescope (SPT) and the {\it Planck} mission. We model this cross-correlation measurement together with the galaxy auto-correlation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure $\langle b_{h}P_{e}\rangle$, using large-scale information. We find $\langle b_{h}P_{e}\rangle$ to be $[0.16^{+0.03}_{-0.04},0.28^{+0.04}_{-0.05},0.45^{+0.06}_{-0.10},0.54^{+0.08}_{-0.07},0.61^{+0.08}_{-0.06},0.63^{+0.07}_{-0.08}]$ meV cm$^{-3}$ at redshifts $z \sim [0.30, 0.46, 0.62,0.77, 0.89, 0.97]$. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of $10^{8.5}$K but are incompatible with the model that assumes an AGN heating temperature of $10^{8.0}$K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within $r_{500c}$ of the galaxies' halos. |
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) CEA/DSM Centre de Saclay (CEA/DSM) Commissariat à l'énergie atomique et aux énergies alternatives (CEA) DES SPT |
format |
Article in Journal/Newspaper |
author |
Omori, Y. Chang, C. Bleem, L.E. Crawford, T. Drlica-Wagner, A. Raghunathan, S. Zacharegkas, G. Abbott, T.M.C. Aguena, M. Alarcon, A. Allam, S. Alves, O. Amon, A. Avila, S. Baxter, E. Bechtol, K. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Brooks, D. Burke, D.L. Campos, A. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Chang, C.L. Chen, A. Choi, A. Chown, R. Costanzi, M. Crites, A.T. Crocce, M. da Costa, L.N. Pereira, M.E.S. de Haan, T. de Vicente, J. Derose, J. Desai, S. Diehl, H.T. Dobbs, M.A. Dodelson, S. Doel, P. Elvin-Poole, J. Everett, W. Everett, S. Ferrero, I. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gatti, M. George, E.M. Gerdes, D.W. Giannini, G. Gruen, D. Gruendl, R.A. Gschwend, J. Gutierrez, G. Halverson, N.W. Hinton, S.R. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hrubes, J.D. James, D.J. Knox, L. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, A.T. Luong-Van, D. Maccrann, N. Marshall, J.L. Mccullough, J. Mcmahon, J.J. Melchior, P. Mena-Fernández, J. Menanteau, F. Miquel, R. Mocanu, L. Mohr, J.J. Muir, J. Myles, J. Natoli, T. Padin, S. Palmese, A. Pandey, S. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A.A. Porredon, A. Pryke, C. Raveri, M. Reichardt, C.L. Rodriguez-Monroy, M. Ross, A.J. Ruhl, J.E. Rykoff, E. Sánchez, C. Sanchez, E. Scarpine, V. Schaffer, K.K. Sevilla-Noarbe, I. Sheldon, E. Shirokoff, E. Smith, M. Soares-Santos, M. Staniszewski, Z. Stark, A.A. Suchyta, E. Tarle, G. Thomas, D. Troxel, M.A. Tucker, D.L. Vieira, J.D. Vincenzi, M. Weaverdyck, N. Williamson, R. Yanny, B. Yin, B. |
author_facet |
Omori, Y. Chang, C. Bleem, L.E. Crawford, T. Drlica-Wagner, A. Raghunathan, S. Zacharegkas, G. Abbott, T.M.C. Aguena, M. Alarcon, A. Allam, S. Alves, O. Amon, A. Avila, S. Baxter, E. Bechtol, K. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Brooks, D. Burke, D.L. Campos, A. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Chang, C.L. Chen, A. Choi, A. Chown, R. Costanzi, M. Crites, A.T. Crocce, M. da Costa, L.N. Pereira, M.E.S. de Haan, T. de Vicente, J. Derose, J. Desai, S. Diehl, H.T. Dobbs, M.A. Dodelson, S. Doel, P. Elvin-Poole, J. Everett, W. Everett, S. Ferrero, I. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gatti, M. George, E.M. Gerdes, D.W. Giannini, G. Gruen, D. Gruendl, R.A. Gschwend, J. Gutierrez, G. Halverson, N.W. Hinton, S.R. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hrubes, J.D. James, D.J. Knox, L. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, A.T. Luong-Van, D. Maccrann, N. Marshall, J.L. Mccullough, J. Mcmahon, J.J. Melchior, P. Mena-Fernández, J. Menanteau, F. Miquel, R. Mocanu, L. Mohr, J.J. Muir, J. Myles, J. Natoli, T. Padin, S. Palmese, A. Pandey, S. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A.A. Porredon, A. Pryke, C. Raveri, M. Reichardt, C.L. Rodriguez-Monroy, M. Ross, A.J. Ruhl, J.E. Rykoff, E. Sánchez, C. Sanchez, E. Scarpine, V. Schaffer, K.K. Sevilla-Noarbe, I. Sheldon, E. Shirokoff, E. Smith, M. Soares-Santos, M. Staniszewski, Z. Stark, A.A. Suchyta, E. Tarle, G. Thomas, D. Troxel, M.A. Tucker, D.L. Vieira, J.D. Vincenzi, M. Weaverdyck, N. Williamson, R. Yanny, B. Yin, B. |
author_sort |
Omori, Y. |
title |
Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck |
title_short |
Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck |
title_full |
Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck |
title_fullStr |
Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck |
title_full_unstemmed |
Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck |
title_sort |
mapping gas around massive galaxies: cross-correlation of des y3 galaxies and compton-$y$-maps from spt and planck |
publisher |
HAL CCSD |
publishDate |
2023 |
url |
https://hal.science/hal-03826315 https://hal.science/hal-03826315/document https://hal.science/hal-03826315/file/stad1167.pdf https://doi.org/10.1093/mnras/stad1167 |
genre |
South pole |
genre_facet |
South pole |
op_source |
Mon.Not.Roy.Astron.Soc. https://hal.science/hal-03826315 Mon.Not.Roy.Astron.Soc., 2023, 522 (2), pp.3163-3182. ⟨10.1093/mnras/stad1167⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2210.08633 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad1167 hal-03826315 https://hal.science/hal-03826315 https://hal.science/hal-03826315/document https://hal.science/hal-03826315/file/stad1167.pdf ARXIV: 2210.08633 doi:10.1093/mnras/stad1167 INSPIRE: 2166164 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1093/mnras/stad1167 |
container_title |
Monthly Notices of the Royal Astronomical Society |
container_volume |
522 |
container_issue |
2 |
container_start_page |
3163 |
op_container_end_page |
3182 |
_version_ |
1796931868026732544 |
spelling |
ftinsu:oai:HAL:hal-03826315v1 2024-04-21T08:11:58+00:00 Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck Omori, Y. Chang, C. Bleem, L.E. Crawford, T. Drlica-Wagner, A. Raghunathan, S. Zacharegkas, G. Abbott, T.M.C. Aguena, M. Alarcon, A. Allam, S. Alves, O. Amon, A. Avila, S. Baxter, E. Bechtol, K. Benson, B.A. Bernstein, G.M. Bertin, E. Bocquet, S. Brooks, D. Burke, D.L. Campos, A. Carlstrom, J.E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Chang, C.L. Chen, A. Choi, A. Chown, R. Costanzi, M. Crites, A.T. Crocce, M. da Costa, L.N. Pereira, M.E.S. de Haan, T. de Vicente, J. Derose, J. Desai, S. Diehl, H.T. Dobbs, M.A. Dodelson, S. Doel, P. Elvin-Poole, J. Everett, W. Everett, S. Ferrero, I. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gatti, M. George, E.M. Gerdes, D.W. Giannini, G. Gruen, D. Gruendl, R.A. Gschwend, J. Gutierrez, G. Halverson, N.W. Hinton, S.R. Holder, G.P. Hollowood, D.L. Holzapfel, W.L. Honscheid, K. Hrubes, J.D. James, D.J. Knox, L. Kuehn, K. Kuropatkin, N. Lahav, O. Lee, A.T. Luong-Van, D. Maccrann, N. Marshall, J.L. Mccullough, J. Mcmahon, J.J. Melchior, P. Mena-Fernández, J. Menanteau, F. Miquel, R. Mocanu, L. Mohr, J.J. Muir, J. Myles, J. Natoli, T. Padin, S. Palmese, A. Pandey, S. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A.A. Porredon, A. Pryke, C. Raveri, M. Reichardt, C.L. Rodriguez-Monroy, M. Ross, A.J. Ruhl, J.E. Rykoff, E. Sánchez, C. Sanchez, E. Scarpine, V. Schaffer, K.K. Sevilla-Noarbe, I. Sheldon, E. Shirokoff, E. Smith, M. Soares-Santos, M. Staniszewski, Z. Stark, A.A. Suchyta, E. Tarle, G. Thomas, D. Troxel, M.A. Tucker, D.L. Vieira, J.D. Vincenzi, M. Weaverdyck, N. Williamson, R. Yanny, B. Yin, B. 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) CEA/DSM Centre de Saclay (CEA/DSM) Commissariat à l'énergie atomique et aux énergies alternatives (CEA) DES SPT 2023 https://hal.science/hal-03826315 https://hal.science/hal-03826315/document https://hal.science/hal-03826315/file/stad1167.pdf https://doi.org/10.1093/mnras/stad1167 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2210.08633 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad1167 hal-03826315 https://hal.science/hal-03826315 https://hal.science/hal-03826315/document https://hal.science/hal-03826315/file/stad1167.pdf ARXIV: 2210.08633 doi:10.1093/mnras/stad1167 INSPIRE: 2166164 info:eu-repo/semantics/OpenAccess Mon.Not.Roy.Astron.Soc. https://hal.science/hal-03826315 Mon.Not.Roy.Astron.Soc., 2023, 522 (2), pp.3163-3182. ⟨10.1093/mnras/stad1167⟩ galaxies: structure large-scale structure of Universe cosmology: observations [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2023 ftinsu https://doi.org/10.1093/mnras/stad1167 2024-04-05T00:27:06Z International audience We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-$y$-maps generated using data from the South Pole Telescope (SPT) and the {\it Planck} mission. We model this cross-correlation measurement together with the galaxy auto-correlation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure $\langle b_{h}P_{e}\rangle$, using large-scale information. We find $\langle b_{h}P_{e}\rangle$ to be $[0.16^{+0.03}_{-0.04},0.28^{+0.04}_{-0.05},0.45^{+0.06}_{-0.10},0.54^{+0.08}_{-0.07},0.61^{+0.08}_{-0.06},0.63^{+0.07}_{-0.08}]$ meV cm$^{-3}$ at redshifts $z \sim [0.30, 0.46, 0.62,0.77, 0.89, 0.97]$. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of $10^{8.5}$K but are incompatible with the model that assumes an AGN heating temperature of $10^{8.0}$K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within $r_{500c}$ of the galaxies' halos. Article in Journal/Newspaper South pole Institut national des sciences de l'Univers: HAL-INSU Monthly Notices of the Royal Astronomical Society 522 2 3163 3182 |