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
| Authors: | ; ; ; ; ; |
|---|---|
| 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 |
| _version_ | 1878732991051595776 |
|---|---|
| author | Cui, Weiguang |
| author2 | Yepes Alonso, Gustavo Knebe, Alexander Akrami, Yashar García-Bellido Capdevila, Juan Euclid Collaboration |
| author2_role | author author author author author |
| author_browse | Akrami, Yashar Cui, Weiguang Euclid Collaboration García-Bellido Capdevila, Juan Knebe, Alexander Yepes Alonso, Gustavo |
| author_facet | Cui, Weiguang Yepes Alonso, Gustavo Knebe, Alexander Akrami, Yashar García-Bellido Capdevila, Juan Euclid Collaboration |
| author_role | author |
| collection | Biblos-e Archivo. Repositorio Institucional de la UAM |
| 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 |
| eu_rights_str_mv | openAccess |
| format | article |
| id | ES_4de7e660d3692387c8e87adca29af2ce |
| institution | Universidad Autónoma de Madrid |
| instname_str | Universidad Autónoma de Madrid |
| language | eng |
| network_acronym_str | ES |
| network_name_str | España |
| oai_identifier_str | oai:repositorio.uam.es:10486/718145 |
| publishDate | 2024 |
| publishDateSort | 2024 |
| publisher | EDP Sciences |
| publisherStr | EDP Sciences |
| reponame_str | Biblos-e Archivo. Repositorio Institucional de la UAM |
| spelling | Euclid preparation: XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations Cui, Weiguang Yepes Alonso, Gustavo Knebe, Alexander Akrami, Yashar García-Bellido Capdevila, Juan Euclid Collaboration Cosmology: theory dark energy dark matter galaxies: clusters: general galaxies: halos large-scale structure of Universe Física 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 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 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 Sciences http://hdl.handle.net/10486/718145 https://dx.doi.org/10.1051/0004-6361/202346058 |
| 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 | 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_short | 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 |
| topic | Cosmology: theory dark energy dark matter galaxies: clusters: general galaxies: halos large-scale structure of Universe Física |
| topic_facet | Cosmology: theory dark energy dark matter galaxies: clusters: general galaxies: halos large-scale structure of Universe Física |
| url | http://hdl.handle.net/10486/718145 https://dx.doi.org/10.1051/0004-6361/202346058 |