Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations

Euclid Collaboration: et al.

Detalles Bibliográficos
Autores: Euclid Collaboration, Castander, Francisco J., Fosalba, Pablo, Serrano, Santiago, Akrami, Yashar, García-Bellido, Juan
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/365803
Acceso en línea:http://hdl.handle.net/10261/365803
Access Level:acceso abierto
Palabra clave:Galaxies: clusters: general
Galaxies: halos
Large-scale structure of Universe
Dark matter
Dark energy
Cosmology: theory
id ES_296aa856c32fbda075bfa18255f5211e
oai_identifier_str oai:digital.csic.es:10261/365803
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
title Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
spellingShingle Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
Euclid Collaboration
Galaxies: clusters: general
Galaxies: halos
Large-scale structure of Universe
Dark matter
Dark energy
Cosmology: theory
title_short Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
title_full Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
title_fullStr Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
title_full_unstemmed Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
title_sort Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations
dc.creator.none.fl_str_mv Euclid Collaboration
Castander, Francisco J.
Fosalba, Pablo
Serrano, Santiago
Akrami, Yashar
García-Bellido, Juan
author Euclid Collaboration
author_facet Euclid Collaboration
Castander, Francisco J.
Fosalba, Pablo
Serrano, Santiago
Akrami, Yashar
García-Bellido, Juan
author_role author
author2 Castander, Francisco J.
Fosalba, Pablo
Serrano, Santiago
Akrami, Yashar
García-Bellido, Juan
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv Ministero dell'Istruzione, dell'Università e della Ricerca
Agenzia Spaziale Italiana
Istituto Nazionale di Astrofisica
Ministerio de Ciencia, Innovación y Universidades (España)
Ministerio de Ciencia e Innovación (España)
Science and Technology Facilities Council (UK)
Agencia Estatal de Investigación (España)
Comunidad de Madrid
Fundação para a Ciência e a Tecnologia (Portugal)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: clusters: general
Galaxies: halos
Large-scale structure of Universe
Dark matter
Dark energy
Cosmology: theory
topic Galaxies: clusters: general
Galaxies: halos
Large-scale structure of Universe
Dark matter
Dark energy
Cosmology: theory
description Euclid Collaboration: et al.
publishDate 2024
dc.date.none.fl_str_mv 2024
2024
2024
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/365803
url http://hdl.handle.net/10261/365803
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
#PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-122603NB-C21
2020-T1/TIC-19882/AtraccióndeTalento-CM
https://doi.org/10.1051/0004-6361/202346058
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869405003222876160
spelling Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulationsEuclid CollaborationCastander, Francisco J.Fosalba, PabloSerrano, SantiagoAkrami, YasharGarcía-Bellido, JuanGalaxies: clusters: generalGalaxies: halosLarge-scale structure of UniverseDark matterDark energyCosmology: theoryEuclid Collaboration: et al.The photometric catalogue of galaxy clusters extracted from ESA Euclid data is expected to be very competitive for cosmological studies. Using dedicated hydrodynamical simulations, we present systematic analyses simulating the expected weak-lensing profiles from clusters in a variety of dynamic states and for a wide range of redshifts. In order to derive cluster masses, we use a model consistent with the implementation within the Euclid Consortium of the dedicated processing function and find that when we jointly model the mass and concentration parameter of the Navarro–Frenk–White halo profile, the weak-lensing masses tend to be biased low by 5–10% on average with respect to the true mass, up to z = 0.5. For a fixed value for the concentration c200 = 3, the mass bias is decreases to lower than 5%, up to z = 0.7, along with the relative uncertainty. Simulating the weak-lensing signal by projecting along the directions of the axes of the moment of inertia tensor ellipsoid, we find that orientation matters: when clusters are oriented along the major axis, the lensing signal is boosted, and the recovered weak-lensing mass is correspondingly overestimated. Typically, the weak-lensing mass bias of individual clusters is modulated by the weak-lensing signal-to-noise ratio, which is related to the redshift evolution of the number of galaxies used for weak-lensing measurements: the negative mass bias tends to be stronger toward higher redshifts. However, when we use a fixed value of the concentration parameter, the redshift evolution trend is reduced. These results provide a solid basis for the weak-lensing mass calibration required by the cosmological application of future cluster surveys from Euclid and Rubin.C.G., M.M., and L.M. acknowledge support from the grant PRIN-MIUR 2017 WSCC32 ZOOMING, and the support from the grant ASI n.2018-23-HH.0. C.G. acknowledges funding from the Italian National Institute of Astrophysics under the grant “Bando PrIN 2019”, PI: Viola Allevato and from the HPC-Europa3 Transnational Access programme HPC17VDILO. G.C. also thanks the support from INAF theory Grant 2022: Illuminating Dark Matter using weak-lensing by Cluster Satellites, PI: Carlo Giocoli. M.M. acknowledges financial support from PRIN-MIUR grant and 2020SKSTHZ, INAF “main-stream” 1.05.01.86.20: “Deep and wide view of galaxy clusters (P.I.: M. Nonino)” and INAF “main-stream” 1.05.01.86.31 “The deepest view of high-redshift galaxies and globular cluster precursors in the early Universe” (P.I.: E. Vanzella). S.B. and M.M. acknowledge financial support from the InDark INFN Grant. G.Y. and A.K. would like to thank the Ministerio de Ciencia e Innovación (Spain) for financial support under research grant PID2021-122603NB-C21. W.C. is supported by the STFC AGP Grant ST/V000594/1 and the Atracción de Talento Contract no. 2020-T1/TIC-19882 granted by the Comunidad de Madrid in Spain. He also thanks the Ministerio de Ciencia e Innovación (Spain) for financial support under Project grant PID2021-122603NB-C21. He further acknowledges the science research grants from the China Manned Space Project with NO. CMS-CSST-2021-A01 and CMS-CSST-2021-B01. We acknowledge the use of computational resources from the parallel computing cluster of the Open Physics Hub (https://site.unibo.it/openphysicshub/en) at the Physics and Astronomy Department in Bologna. T.S. acknowledges support from FFG grant number 899537. C.J.M. acknowledges FCT and POCH/FSE (EC) support through Investigador FCT Contract 2021.01214.CEECIND/CP1658/CT0001.Peer reviewedEDP SciencesMinistero dell'Istruzione, dell'Università e della RicercaAgenzia Spaziale ItalianaIstituto Nazionale di AstrofisicaMinisterio de Ciencia, Innovación y Universidades (España)Ministerio de Ciencia e Innovación (España)Science and Technology Facilities Council (UK)Agencia Estatal de Investigación (España)Comunidad de MadridFundação para a Ciência e a Tecnologia (Portugal)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/365803reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-122603NB-C212020-T1/TIC-19882/AtraccióndeTalento-CMhttps://doi.org/10.1051/0004-6361/202346058Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3658032026-05-22T06:33:51Z
score 15.81155

Similares en LA Referencia