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Spatially resolved stellar populations of 0.3 < z < 6.0 galaxies in WHL 0137-08 and MACS 0647+70 clusters as revealed by JWST: How Do galaxies grow and quench over cosmic time?

dc.contributor.authorAbdurro'uf
dc.contributor.authorCoe, Dan
dc.contributor.authorJung, Intae
dc.contributor.authorFerguson, Henry C.
dc.contributor.authorBrammer, Gabriel
dc.contributor.authorIyer, Kartheik G.
dc.contributor.authorBradley, Larry D.
dc.contributor.authorDayal, Pratika
dc.contributor.authorWindhorst, Rogier A.
dc.contributor.authorZitrin, Adi
dc.contributor.authorMeena, Ashish Kumar
dc.contributor.authorOguri, Masamune
dc.contributor.authorDiego Rodríguez, José María 
dc.contributor.authorKokorev, Vasily
dc.contributor.authorDimauro, Paola
dc.contributor.authorAdamo, Angela
dc.contributor.authorConselice, Christopher J.
dc.contributor.authorWelch, Brian
dc.contributor.authorVanzella, Eros
dc.contributor.authorHsiao, Tiger Yu-Yang
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-02-01T13:21:57Z
dc.date.available2024-02-01T13:21:57Z
dc.date.issued2023
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttps://hdl.handle.net/10902/31382
dc.description.sponsorshipWe thank the anonymous referee for providing valuable comments that helped to improve this paper. We thank Takahiro Morishita for the useful discussion and comments. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope (JWST). Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. The specific observations analyzed can be accessed via doi:10.17909/d2er-wq71 and doi:10.17909/cqfq 5n80. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS526555. Support to MAST for these data is provided by the NASA Office of Space Science via grant NAG57584 and by other grants and contracts. A. and T.H. are funded by a grant for JWST-GO-01433 provided by STScI under NASA contract NAS5-03127. The CosmicDawn Center is funded by the Danish National Research Foundation (DNRF) under grant #140. P.D. acknowledges support from the NWO grant 016.VIDI.189.162 (“ODIN”) and from the European Commission’s and University of Groningen’s CO-FUND Rosalind Franklin program. R.A.W. acknowledges support from NASA JWST Interdisciplinary Scientist grants NAG5-12460, NNX14AN10G, and 80NSSC18K0200 from GSFC. A.Z. and A.K.M. acknowledge support by grant 2020750 from the United States–Israel Binational Science Foundation (BSF) and grant 2109066 from the United States National Science Foundation (NSF), and by the Ministry of Science & Technology, Israel. M.O. acknowledges support from JSPS KAKENHI grant Nos. JP22H01260, JP20H05856, JP20H00181, and JP22K21349. A.A. acknowl edges support from the Swedish Research Council (Vetenskapsrådet project grants 2021-05559). E.V. acknowledges financial support through grants PRIN-MIUR 2017WSCC32, 2020SKSTHZ, and the INAF GO Grant 2022 (P.I. E.Vanzella).es_ES
dc.format.extent24 p.es_ES
dc.language.isoenges_ES
dc.publisherInstitute of Physics Publishinges_ES
dc.rightsAttribution 4.0 Internationales_ES
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourceAstrophysical Journal, 2023, 945(2), 117es_ES
dc.subject.otherGalaxy evolutiones_ES
dc.subject.otherGalaxy formationes_ES
dc.subject.otherGalaxy clusterses_ES
dc.subject.otherGalaxy quenchinges_ES
dc.titleSpatially resolved stellar populations of 0.3 < z < 6.0 galaxies in WHL 0137-08 and MACS 0647+70 clusters as revealed by JWST: How Do galaxies grow and quench over cosmic time?es_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.3847/1538-4357/acba06es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.3847/1538-4357/acba06
dc.type.versionpublishedVersiones_ES


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