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

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

Bibliographic Details
Authors: Cui, Weiguang, Yepes Alonso, Gustavo, Knebe, Alexander, Akrami, Yashar, García-Bellido Capdevila, Juan, Euclid Collaboration
Format: article
Publication Date:2024
Country:España
Institution:Universidad Autónoma de Madrid
Repository:Biblos-e Archivo. Repositorio Institucional de la UAM
Language:English
OAI Identifier:oai:repositorio.uam.es:10486/718145
Online Access:http://hdl.handle.net/10486/718145
https://dx.doi.org/10.1051/0004-6361/202346058
Access Level:Open access
Keyword:Cosmology: theory
dark energy
dark matter
galaxies: clusters: general
galaxies: halos
large-scale structure of Universe
Física
id ES_4de7e660d3692387c8e87adca29af2ce
oai_identifier_str oai:repositorio.uam.es:10486/718145
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
Cui, Weiguang
Cosmology: theory
dark energy
dark matter
galaxies: clusters: general
galaxies: halos
large-scale structure of Universe
Física
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 Cui, Weiguang
Yepes Alonso, Gustavo
Knebe, Alexander
Akrami, Yashar
García-Bellido Capdevila, Juan
Euclid Collaboration
author Cui, Weiguang
author_facet Cui, Weiguang
Yepes Alonso, Gustavo
Knebe, Alexander
Akrami, Yashar
García-Bellido Capdevila, Juan
Euclid Collaboration
author_role author
author2 Yepes Alonso, Gustavo
Knebe, Alexander
Akrami, Yashar
García-Bellido Capdevila, Juan
Euclid Collaboration
author2_role author
author
author
author
author
dc.contributor.none.fl_str_mv Departamento de Física Teórica
Facultad de Ciencias
dc.subject.none.fl_str_mv Cosmology: theory
dark energy
dark matter
galaxies: clusters: general
galaxies: halos
large-scale structure of Universe
Física
topic Cosmology: theory
dark energy
dark matter
galaxies: clusters: general
galaxies: halos
large-scale structure of Universe
Física
description Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-01-16
dc.type.none.fl_str_mv research article
http://purl.org/coar/resource_type/c_2df8fbb1
VoR
http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv http://hdl.handle.net/10486/718145
https://dx.doi.org/10.1051/0004-6361/202346058
url http://hdl.handle.net/10486/718145
https://dx.doi.org/10.1051/0004-6361/202346058
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
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:Biblos-e Archivo. Repositorio Institucional de la UAM
instname:Universidad Autónoma de Madrid
instname_str Universidad Autónoma de Madrid
reponame_str Biblos-e Archivo. Repositorio Institucional de la UAM
collection Biblos-e Archivo. Repositorio Institucional de la UAM
repository.name.fl_str_mv
repository.mail.fl_str_mv
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spelling Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulationsCui, WeiguangYepes Alonso, GustavoKnebe, AlexanderAkrami, YasharGarcía-Bellido Capdevila, JuanEuclid CollaborationCosmology: theorydark energydark mattergalaxies: clusters: generalgalaxies: haloslarge-scale structure of UniverseFísicaArtículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAMThe 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 RubinC.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 highredshift 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. The THREE HUNDRED simulations used in this work have been performed in the MareNostrum Supercomputer at the Barcelona Supercomputing Center, thanks to CPU time granted by the Red Española de Supercomputación. W.C. is sup ported 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 sup port 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 compu tational resources from the parallel computing cluster of the Open Physics Hub (https://site.unibo.it/openphysicshub/en) at the Physics and Astron omy Department in Bologna. T.S. acknowledges support from FFG grant num ber 899537. C.J.M. acknowledges FCT and POCH/FSE (EC) support through Investigador FCT Contract 2021.01214.CEECIND/CP1658/CT0001. The fig ures with the corner plots displaying the posterior distributions have been pro duced using the package pygtc developed by Bocquet & Carter (2016). The authors acknowledge the Euclid Consortium, the European Space Agency, and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the French Cen tre National d’Etudes Spatiales, the Deutsches Zentrum für Luft- und Raum fahrt, the Danish Space Research Institute, the Fundação para a Ciência e a Tecnologia, the Ministerio de Ciencia e Innovación, the National Aeronautics and Space Administration, the National Astronomical Observatory of Japan, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid web site (http://www.euclid-ec.org)EDP SciencesDepartamento de Física TeóricaFacultad de Ciencias20242024-01-16research articlehttp://purl.org/coar/resource_type/c_2df8fbb1VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10486/718145https://dx.doi.org/10.1051/0004-6361/202346058reponame:Biblos-e Archivo. Repositorio Institucional de la UAMinstname:Universidad Autónoma de MadridInglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:repositorio.uam.es:10486/7181452026-06-23T12:46:27Z
score 15.812429

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