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dc.contributor.authorSocolovsky, Miguel
dc.contributor.authorAlmaini, Omar
dc.contributor.authorHatch, Nina A.
dc.contributor.authorWild, Vivienne
dc.contributor.authorMaltby, David T.
dc.contributor.authorHartley, William G.
dc.contributor.authorSimpson, Chris
dc.date.accessioned2018-02-13T09:32:41Z
dc.date.available2018-02-13T09:32:41Z
dc.date.issued2018-05
dc.identifier252233953
dc.identifier000a1307-2226-40da-beca-308dd678ba10
dc.identifier85052431454
dc.identifier000429276700097
dc.identifier.citationSocolovsky , M , Almaini , O , Hatch , N A , Wild , V , Maltby , D T , Hartley , W G & Simpson , C 2018 , ' The enhancement of rapidly quenched galaxies in distant clusters at 0.5 < z < 1.0 ' , Monthly Notices of the Royal Astronomical Society , vol. 476 , no. 1 , pp. 1242-1257 . https://doi.org/10.1093/mnras/sty312en
dc.identifier.issn0035-8711
dc.identifier.otherBibCode: 2018arXiv180201593S
dc.identifier.urihttps://hdl.handle.net/10023/12708
dc.descriptionFunding: MS acknowledges support from IAC and STFC. VW acknowledges support from the European Research Council Starting grant (SEDmorph, P.I. V. Wild).en
dc.description.abstractWe investigate the relationship between environment and galaxy evolution in the redshift range 0.5 < z < 1.0. Galaxy overdensities are selected using a Friends-of-Friends algorithm, applied to deep photometric data in the Ultra-Deep Survey (UDS) field. A study of the resulting stellar mass functions reveals clear differences between cluster and field environments, with a strong excess of low-mass rapidly quenched galaxies in cluster environments compared to the field. Cluster environments also show a corresponding deficit of young, low-mass star-forming galaxies, which show a sharp radial decline towards cluster centres. By comparing mass functions and radial distributions, we conclude that young star-forming galaxies are rapidly quenched as they enter overdense environments, becoming post-starburst galaxies before joining the red sequence. Our results also point to the existence of two environmental quenching pathways operating in galaxy clusters, operating on different timescales. Fast quenching acts on galaxies with high specific star-formation rates, operating on timescales shorter than the cluster dynamical time ( < 1 Gyr). In contrast, slow quenching affects galaxies with moderate specific star-formation rates, regardlessof their stellar mass, and acts on longer timescales (≳ 1 Gyr). Of the cluster galaxies in the stellar mass range 9.0 < log(M/M⊙) < 10.5 quenched during this epoch, we find that 73% were transformed through fast quenching, while the remaining 27% followed the slow quenching route.
dc.format.extent1622467
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: quenchingen
dc.subjectGalaxies: environment, clustersen
dc.subjectGalaxies: high-redshiften
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe enhancement of rapidly quenched galaxies in distant clusters at 0.5 < z < 1.0en
dc.typeJournal articleen
dc.contributor.sponsorEuropean Research Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/mnras/sty312
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2018arXiv180201593Sen
dc.identifier.grantnumberERC-2012-StG-20111012en


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