Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.105.123526 http://hdl.handle.net/11449/241393 |
Resumo: | Hot, ionized gas leaves an imprint on the cosmic microwave background via the thermal Sunyaev-Zel'dovich (tSZ) effect. The cross-correlation of gravitational lensing (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) is a powerful probe of the thermal state of ionized baryons throughout the Universe and is sensitive to effects such as baryonic feedback. In a companion paper (Gatti et al. Phys. Rev. D 105, 123525 (2022)PRVDAQ2470-0010), we present tomographic measurements and validation tests of the cross-correlation between Galaxy shear measurements from the first three years of observations of the Dark Energy Survey and tSZ measurements from a combination of Atacama Cosmology Telescope and Planck observations. In this work, we use the same measurements to constrain models for the pressure profiles of halos across a wide range of halo mass and redshift. We find evidence for reduced pressure in low-mass halos, consistent with predictions for the effects of feedback from active Galactic nuclei. We infer the hydrostatic mass bias (BM500c/MSZ) from our measurements, finding B=1.8±0.1 when adopting the Planck-preferred cosmological parameters. We additionally find that our measurements are consistent with a nonzero redshift evolution of B, with the correct sign and sufficient magnitude to explain the mass bias necessary to reconcile cluster count measurements with the Planck-preferred cosmology. Our analysis introduces a model for the impact of intrinsic alignments (IAs) of galaxy shapes on the shear-tSZ correlation. We show that IA can have a significant impact on these correlations at current noise levels. |
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spelling |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profilesHot, ionized gas leaves an imprint on the cosmic microwave background via the thermal Sunyaev-Zel'dovich (tSZ) effect. The cross-correlation of gravitational lensing (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) is a powerful probe of the thermal state of ionized baryons throughout the Universe and is sensitive to effects such as baryonic feedback. In a companion paper (Gatti et al. Phys. Rev. D 105, 123525 (2022)PRVDAQ2470-0010), we present tomographic measurements and validation tests of the cross-correlation between Galaxy shear measurements from the first three years of observations of the Dark Energy Survey and tSZ measurements from a combination of Atacama Cosmology Telescope and Planck observations. In this work, we use the same measurements to constrain models for the pressure profiles of halos across a wide range of halo mass and redshift. We find evidence for reduced pressure in low-mass halos, consistent with predictions for the effects of feedback from active Galactic nuclei. We infer the hydrostatic mass bias (BM500c/MSZ) from our measurements, finding B=1.8±0.1 when adopting the Planck-preferred cosmological parameters. We additionally find that our measurements are consistent with a nonzero redshift evolution of B, with the correct sign and sufficient magnitude to explain the mass bias necessary to reconcile cluster count measurements with the Planck-preferred cosmology. Our analysis introduces a model for the impact of intrinsic alignments (IAs) of galaxy shapes on the shear-tSZ correlation. We show that IA can have a significant impact on these correlations at current noise levels.Department of Physics and Astronomy University of PennsylvaniaInstitute for Astronomy University of Hawai'i, 2680 Woodlawn DriveDepartment of Physics Columbia UniversityCenter for Computational Astrophysics Flatiron InstituteDepartment of Astronomy/Steward Observatory University of Arizona, 933 North Cherry AvenueInstitut de Física d'Altes Energies (IFAE) The Barcelona Institute of Science and Technology Campus UAB, BellaterraLawrence Berkeley National Laboratory, 1 Cyclotron RoadDepartment of Physics University of ArizonaDepartment of Astronomy Cornell UniversityArgonne National Laboratory, 9700 South Cass AvenueKavli Institute for Particle Astrophysics and Cosmology Stanford University, P. O. Box 2450Department of Physics Carnegie Mellon UniversityDepartment of Astronomy and Astrophysics University of ChicagoKavli Institute for Cosmological Physics University of ChicagoDepartment of Physics Duke UniversityCenter for Cosmology and Astro-Particle Physics The Ohio State UniversityDepartment of Physics The Ohio State UniversitySanta Cruz Institute for Particle PhysicsJet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove DriveDepartment of Physics University of Oxford, Denys Wilkinson Building, Keble RoadJodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford RoadDepartment of Applied Mathematics and Theoretical Physics University of CambridgeDepartment of Physics Stanford University, 382 Via Pueblo MallSLAC National Accelerator LaboratoryInstituto de Física Gleb Wataghin Universidade Estadual de Campinas, São PauloInstitut d'Estudis Espacials de Catalunya (IEEC)Institute of Space Sciences (ICE CSIC), Campus UAB, Carrer de Can MagransLaboratório Interinstitucional de E-Astronomia - LIneA, Rua Gal. José Cristino 77, RJFermi National Accelerator Laboratory, P. O. Box 500Instituto de Física Teórica Universidade Estadual PaulistaCNRS UMR 7095 Institut d'Astrophysique de ParisSorbonne Universités UPMC University Paris 06 UMR 7095 Institut d'Astrophysique de ParisCanadian Institute for Theoretical Astrophysics University of Toronto, 60 St. George StreetDepartment of Physics and Astronomy University College London, Gower StreetSchool of Physics and Astronomy Cardiff University, The ParadeInstituto de Astrofisica de Canarias, TenerifeUniversidad de la Laguna Departamento Astrofísica, TenerifeCenter for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark StreetDepartment of Astronomy University of Illinois at Urbana-Champaign, 1002 West Green StreetPhysics Department University of Wisconsin-Madison, 2320 Chamberlin Hall, 1150 University AvenueAstronomy Unit Department of Physics University of Trieste, via Tiepolo 11INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11Institute for Fundamental Physics of the Universe, Via Beirut 2Observatório Nacional, Rua Gal. José Cristino 77, RJDepartment of Physics University of MichiganCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Department of Physics IIT Hyderabad, TelanganaFaculty of Physics Ludwig-Maximilians-Universität, Scheinerstrasse 1Department of Astrophysical Sciences Princeton University, Peyton HallDepartment of Physics Princeton University, Jadwin HallDepartment of Astronomy University of MichiganLawrence-Berkeley National Laboratory, One Cyclotron RoadBerkeley Center for Cosmological Physics University of CaliforniaInstitute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 BlindernInstituto de Fisica Teorica UAM/CSIC Universidad Autonoma de MadridInstitute of Astronomy University of Cambridge, Madingley RoadKavli Institute for Cosmology University of Cambridge, Madingley RoadDavid A. Dunlap Department of Astronomy and Astrophysics University of Toronto, 50 St. George StreetSchool of Mathematics and Physics University of QueenslandDepartment of Physics and Astronomy Rutgers University, 136 Frelinghuysen RoadCenter for Astrophysics | Harvard and Smithsonian, 60 Garden StreetAustralian Astronomical Optics Macquarie UniversityLowell Observatory, 1400 Mars Hill RoadDepartamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318, SPDunlap Institute of Astronomy and Astrophysics, 50 St. George StreetPerimeter Institute for Theoretical Physics, 31 Caroline Street NorthDepartment of Physics University of ChicagoEnrico Fermi Institute University of ChicagoInstitució Catalana de Recerca i Estudis AvanćatsMax Planck Institute for Extraterrestrial Physics, GiessenbachstrasseAstrophysics Research Centre University of KwaZulu-Natal, Westville CampusSchool of Mathematics Statistics and Computer Science University of KwaZulu-Natal, Westville CampusDepartment of Physics University of Milano-Bicocca, Piazza della Scienza 3, (MI)Kavli Institute at Cornell for Nanoscale Science Cornell UniversityDepartment of Physics and Astronomy University of Sussex, Pevensey BuildingBerkeley Center for Cosmological Physics University of BerkeleyBrookhaven National Laboratory Building 510 Upton New York 11973Instituto de Física Pontificia Universidad Católica de Valparaíso, Casilla 4059School of Physics and Astronomy University of SouthamptonDepartment of Astrophysical Sciences Princeton-UniversityComputer Science and Mathematics Division Oak Ridge National LaboratoryInstitute of Cosmology and Gravitation University of PortsmouthUniversitäts-Sternwarte Fakultät für Physik Ludwig-Maximilians Universität München, Scheinerstrasse 1NASA Goddard Space Flight Center, 8800 Greenbelt RoadMIT Kavli Institute Massachusetts Institute of Technology, 77 Massachusetts AvenueInstituto de Física Teórica Universidade Estadual PaulistaUniversity of PennsylvaniaUniversity of Hawai'iColumbia UniversityFlatiron InstituteUniversity of ArizonaThe Barcelona Institute of Science and TechnologyLawrence Berkeley National LaboratoryCornell UniversityArgonne National LaboratoryStanford UniversityCarnegie Mellon UniversityUniversity of ChicagoDuke UniversityThe Ohio State UniversitySanta Cruz Institute for Particle PhysicsCalifornia Institute of TechnologyUniversity of OxfordUniversity of ManchesterUniversity of CambridgeSLAC National Accelerator LaboratoryUniversidade Estadual de Campinas (UNICAMP)Institut d'Estudis Espacials de Catalunya (IEEC)CSIC)Laboratório Interinstitucional de E-Astronomia - LIneAFermi National Accelerator LaboratoryUniversidade Estadual Paulista (UNESP)Institut d'Astrophysique de ParisUniversity of TorontoUniversity College LondonCardiff UniversityInstituto de Astrofisica de CanariasUniversidad de la LagunaNational Center for Supercomputing ApplicationsUniversity of Illinois at Urbana-ChampaignUniversity of Wisconsin-MadisonUniversity of TriesteINAF-Osservatorio Astronomico di TriesteInstitute for Fundamental Physics of the UniverseObservatório NacionalUniversity of MichiganMedioambientales y Tecnológicas (CIEMAT)IIT HyderabadLudwig-Maximilians-UniversitätPrinceton UniversityLawrence-Berkeley National LaboratoryUniversity of CaliforniaUniversity of OsloUniversidad Autonoma de MadridUniversity of QueenslandRutgers UniversityCenter for Astrophysics | Harvard and SmithsonianMacquarie UniversityLowell ObservatoryUniversidade de São Paulo (USP)Dunlap Institute of Astronomy and AstrophysicsPerimeter Institute for Theoretical PhysicsInstitució Catalana de Recerca i Estudis AvanćatsMax Planck Institute for Extraterrestrial PhysicsUniversity of KwaZulu-NatalUniversity of Milano-BicoccaUniversity of SussexUniversity of BerkeleyNew York 11973Pontificia Universidad Católica de ValparaísoUniversity of SouthamptonPrinceton-UniversityOak Ridge National LaboratoryUniversity of PortsmouthLudwig-Maximilians Universität MünchenNASA Goddard Space Flight CenterMassachusetts Institute of TechnologyPandey, S.Gatti, M.Baxter, E.Hill, J. C.Fang, X.Doux, C.Giannini, G.Raveri, M.Derose, J.Huang, H.Moser, E.Battaglia, N.Alarcon, A.Amon, A.Becker, M.Campos, A.Chang, C.Chen, R.Choi, A.Eckert, K.Elvin-Poole, J.Everett, S.Ferte, A.Harrison, I.Maccrann, N.McCullough, J.Myles, J.Navarro Alsina, A.Prat, J.Rollins, R. P.Sanchez, C.Shin, T.Troxel, M.Tutusaus, I.Yin, B.Aguena, M.Allam, S.Andrade-Oliveira, F. [UNESP]Bernstein, G. M.Bertin, E.Bolliet, B.Bond, J. R.Brooks, D.Calabrese, E.Carnero Rosell, A.Carrasco Kind, M.Carretero, J.Cawthon, R.Costanzi, M.Crocce, M.Da Costa, L. N.Pereira, M. E.S.De Vicente, J.Desai, S.Diehl, H. T.Dietrich, J. P.Doel, P.Dunkley, J.Evrard, A. E.Ferraro, S.Ferrero, I.Flaugher, B.Fosalba, P.García-Bellido, J.Gaztanaga, E.Gerdes, D. W.Giannantonio, T.Gruen, D.Gruendl, R. A.Gschwend, J.Gutierrez, G.Herner, K.Hincks, A. D.Hinton, S. R.Hollowood, D. L.Honscheid, K.Hughes, J. P.Huterer, D.Jain, B.James, D. J.Jeltema, T.Krause, E.Kuehn, K.Lahav, O.Lima, M.Lokken, M.Madhavacheril, M. S.Maia, M. A.G.McMahon, J. J.Melchior, P.Menanteau, F.Miquel, R.Mohr, J. J.Moodley, K.Morgan, R.Nati, F.Niemack, M. D.Page, L.Palmese, A.Paz-Chinchón, F.Pieres, A.Plazas Malagón, A. A.Rodriguez-Monroy, M.Romer, A. K.Sanchez, E.Scarpine, V.Schaan, E.Serrano, S.Sevilla-Noarbe, I.Sheldon, E.Sherwin, B. D.Sifón, C.Smith, M.Soares-Santos, M.Spergel, D.Suchyta, E.Swanson, M. E.C.Tarle, G.Thomas, D.To, C.Varga, T. N.Weller, J.Wollack, E. J.Xu, Z.2023-03-01T21:00:03Z2023-03-01T21:00:03Z2022-06-15info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.105.123526Physical Review D, v. 105, n. 12, 2022.2470-00292470-0010http://hdl.handle.net/11449/24139310.1103/PhysRevD.105.1235262-s2.0-85134653797Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2023-03-01T21:00:06Zoai:repositorio.unesp.br:11449/241393Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-03-01T21:00:06Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
title |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
spellingShingle |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles Pandey, S. |
title_short |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
title_full |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
title_fullStr |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
title_full_unstemmed |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
title_sort |
Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles |
author |
Pandey, S. |
author_facet |
Pandey, S. Gatti, M. Baxter, E. Hill, J. C. Fang, X. Doux, C. Giannini, G. Raveri, M. Derose, J. Huang, H. Moser, E. Battaglia, N. Alarcon, A. Amon, A. Becker, M. Campos, A. Chang, C. Chen, R. Choi, A. Eckert, K. Elvin-Poole, J. Everett, S. Ferte, A. Harrison, I. Maccrann, N. McCullough, J. Myles, J. Navarro Alsina, A. Prat, J. Rollins, R. P. Sanchez, C. Shin, T. Troxel, M. Tutusaus, I. Yin, B. Aguena, M. Allam, S. Andrade-Oliveira, F. [UNESP] Bernstein, G. M. Bertin, E. Bolliet, B. Bond, J. R. Brooks, D. Calabrese, E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cawthon, R. Costanzi, M. Crocce, M. Da Costa, L. N. Pereira, M. E.S. De Vicente, J. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Dunkley, J. Evrard, A. E. Ferraro, S. Ferrero, I. Flaugher, B. Fosalba, P. García-Bellido, J. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Gruen, D. Gruendl, R. A. Gschwend, J. Gutierrez, G. Herner, K. Hincks, A. D. Hinton, S. R. Hollowood, D. L. Honscheid, K. Hughes, J. P. Huterer, D. Jain, B. James, D. J. Jeltema, T. Krause, E. Kuehn, K. Lahav, O. Lima, M. Lokken, M. Madhavacheril, M. S. Maia, M. A.G. McMahon, J. J. Melchior, P. Menanteau, F. Miquel, R. Mohr, J. J. Moodley, K. Morgan, R. Nati, F. Niemack, M. D. Page, L. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Rodriguez-Monroy, M. Romer, A. K. Sanchez, E. Scarpine, V. Schaan, E. Serrano, S. Sevilla-Noarbe, I. Sheldon, E. Sherwin, B. D. Sifón, C. Smith, M. Soares-Santos, M. Spergel, D. Suchyta, E. Swanson, M. E.C. Tarle, G. Thomas, D. To, C. Varga, T. N. Weller, J. Wollack, E. J. Xu, Z. |
author_role |
author |
author2 |
Gatti, M. Baxter, E. Hill, J. C. Fang, X. Doux, C. Giannini, G. Raveri, M. Derose, J. Huang, H. Moser, E. Battaglia, N. Alarcon, A. Amon, A. Becker, M. Campos, A. Chang, C. Chen, R. Choi, A. Eckert, K. Elvin-Poole, J. Everett, S. Ferte, A. Harrison, I. Maccrann, N. McCullough, J. Myles, J. Navarro Alsina, A. Prat, J. Rollins, R. P. Sanchez, C. Shin, T. Troxel, M. Tutusaus, I. Yin, B. Aguena, M. Allam, S. Andrade-Oliveira, F. [UNESP] Bernstein, G. M. Bertin, E. Bolliet, B. Bond, J. R. Brooks, D. Calabrese, E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cawthon, R. Costanzi, M. Crocce, M. Da Costa, L. N. Pereira, M. E.S. De Vicente, J. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Dunkley, J. Evrard, A. E. Ferraro, S. Ferrero, I. Flaugher, B. Fosalba, P. García-Bellido, J. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Gruen, D. Gruendl, R. A. Gschwend, J. Gutierrez, G. Herner, K. Hincks, A. D. Hinton, S. R. Hollowood, D. L. Honscheid, K. Hughes, J. P. Huterer, D. Jain, B. James, D. J. Jeltema, T. Krause, E. Kuehn, K. Lahav, O. Lima, M. Lokken, M. Madhavacheril, M. S. Maia, M. A.G. McMahon, J. J. Melchior, P. Menanteau, F. Miquel, R. Mohr, J. J. Moodley, K. Morgan, R. Nati, F. Niemack, M. D. Page, L. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Rodriguez-Monroy, M. Romer, A. K. Sanchez, E. Scarpine, V. Schaan, E. Serrano, S. Sevilla-Noarbe, I. Sheldon, E. Sherwin, B. D. Sifón, C. Smith, M. Soares-Santos, M. Spergel, D. Suchyta, E. Swanson, M. E.C. Tarle, G. Thomas, D. To, C. Varga, T. N. Weller, J. Wollack, E. J. Xu, Z. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.contributor.none.fl_str_mv |
University of Pennsylvania University of Hawai'i Columbia University Flatiron Institute University of Arizona The Barcelona Institute of Science and Technology Lawrence Berkeley National Laboratory Cornell University Argonne National Laboratory Stanford University Carnegie Mellon University University of Chicago Duke University The Ohio State University Santa Cruz Institute for Particle Physics California Institute of Technology University of Oxford University of Manchester University of Cambridge SLAC National Accelerator Laboratory Universidade Estadual de Campinas (UNICAMP) Institut d'Estudis Espacials de Catalunya (IEEC) CSIC) Laboratório Interinstitucional de E-Astronomia - LIneA Fermi National Accelerator Laboratory Universidade Estadual Paulista (UNESP) Institut d'Astrophysique de Paris University of Toronto University College London Cardiff University Instituto de Astrofisica de Canarias Universidad de la Laguna National Center for Supercomputing Applications University of Illinois at Urbana-Champaign University of Wisconsin-Madison University of Trieste INAF-Osservatorio Astronomico di Trieste Institute for Fundamental Physics of the Universe Observatório Nacional University of Michigan Medioambientales y Tecnológicas (CIEMAT) IIT Hyderabad Ludwig-Maximilians-Universität Princeton University Lawrence-Berkeley National Laboratory University of California University of Oslo Universidad Autonoma de Madrid University of Queensland Rutgers University Center for Astrophysics | Harvard and Smithsonian Macquarie University Lowell Observatory Universidade de São Paulo (USP) Dunlap Institute of Astronomy and Astrophysics Perimeter Institute for Theoretical Physics Institució Catalana de Recerca i Estudis Avanćats Max Planck Institute for Extraterrestrial Physics University of KwaZulu-Natal University of Milano-Bicocca University of Sussex University of Berkeley New York 11973 Pontificia Universidad Católica de Valparaíso University of Southampton Princeton-University Oak Ridge National Laboratory University of Portsmouth Ludwig-Maximilians Universität München NASA Goddard Space Flight Center Massachusetts Institute of Technology |
dc.contributor.author.fl_str_mv |
Pandey, S. Gatti, M. Baxter, E. Hill, J. C. Fang, X. Doux, C. Giannini, G. Raveri, M. Derose, J. Huang, H. Moser, E. Battaglia, N. Alarcon, A. Amon, A. Becker, M. Campos, A. Chang, C. Chen, R. Choi, A. Eckert, K. Elvin-Poole, J. Everett, S. Ferte, A. Harrison, I. Maccrann, N. McCullough, J. Myles, J. Navarro Alsina, A. Prat, J. Rollins, R. P. Sanchez, C. Shin, T. Troxel, M. Tutusaus, I. Yin, B. Aguena, M. Allam, S. Andrade-Oliveira, F. [UNESP] Bernstein, G. M. Bertin, E. Bolliet, B. Bond, J. R. Brooks, D. Calabrese, E. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Cawthon, R. Costanzi, M. Crocce, M. Da Costa, L. N. Pereira, M. E.S. De Vicente, J. Desai, S. Diehl, H. T. Dietrich, J. P. Doel, P. Dunkley, J. Evrard, A. E. Ferraro, S. Ferrero, I. Flaugher, B. Fosalba, P. García-Bellido, J. Gaztanaga, E. Gerdes, D. W. Giannantonio, T. Gruen, D. Gruendl, R. A. Gschwend, J. Gutierrez, G. Herner, K. Hincks, A. D. Hinton, S. R. Hollowood, D. L. Honscheid, K. Hughes, J. P. Huterer, D. Jain, B. James, D. J. Jeltema, T. Krause, E. Kuehn, K. Lahav, O. Lima, M. Lokken, M. Madhavacheril, M. S. Maia, M. A.G. McMahon, J. J. Melchior, P. Menanteau, F. Miquel, R. Mohr, J. J. Moodley, K. Morgan, R. Nati, F. Niemack, M. D. Page, L. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Rodriguez-Monroy, M. Romer, A. K. Sanchez, E. Scarpine, V. Schaan, E. Serrano, S. Sevilla-Noarbe, I. Sheldon, E. Sherwin, B. D. Sifón, C. Smith, M. Soares-Santos, M. Spergel, D. Suchyta, E. Swanson, M. E.C. Tarle, G. Thomas, D. To, C. Varga, T. N. Weller, J. Wollack, E. J. Xu, Z. |
description |
Hot, ionized gas leaves an imprint on the cosmic microwave background via the thermal Sunyaev-Zel'dovich (tSZ) effect. The cross-correlation of gravitational lensing (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) is a powerful probe of the thermal state of ionized baryons throughout the Universe and is sensitive to effects such as baryonic feedback. In a companion paper (Gatti et al. Phys. Rev. D 105, 123525 (2022)PRVDAQ2470-0010), we present tomographic measurements and validation tests of the cross-correlation between Galaxy shear measurements from the first three years of observations of the Dark Energy Survey and tSZ measurements from a combination of Atacama Cosmology Telescope and Planck observations. In this work, we use the same measurements to constrain models for the pressure profiles of halos across a wide range of halo mass and redshift. We find evidence for reduced pressure in low-mass halos, consistent with predictions for the effects of feedback from active Galactic nuclei. We infer the hydrostatic mass bias (BM500c/MSZ) from our measurements, finding B=1.8±0.1 when adopting the Planck-preferred cosmological parameters. We additionally find that our measurements are consistent with a nonzero redshift evolution of B, with the correct sign and sufficient magnitude to explain the mass bias necessary to reconcile cluster count measurements with the Planck-preferred cosmology. Our analysis introduces a model for the impact of intrinsic alignments (IAs) of galaxy shapes on the shear-tSZ correlation. We show that IA can have a significant impact on these correlations at current noise levels. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-06-15 2023-03-01T21:00:03Z 2023-03-01T21:00:03Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevD.105.123526 Physical Review D, v. 105, n. 12, 2022. 2470-0029 2470-0010 http://hdl.handle.net/11449/241393 10.1103/PhysRevD.105.123526 2-s2.0-85134653797 |
url |
http://dx.doi.org/10.1103/PhysRevD.105.123526 http://hdl.handle.net/11449/241393 |
identifier_str_mv |
Physical Review D, v. 105, n. 12, 2022. 2470-0029 2470-0010 10.1103/PhysRevD.105.123526 2-s2.0-85134653797 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1797789609835364352 |