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dc.contributor.authorCheale, R.~A.
dc.contributor.authorGeach, J.~E.
dc.contributor.authorEdge, A.~C.
dc.contributor.authorBlain, A.~W.
dc.contributor.authorChapman, S.~C.
dc.contributor.authorEgami, E.
dc.contributor.authorHogan, M.~T.
dc.contributor.authorRawle, T.~D.
dc.contributor.authorWebb, T.~M.~A.
dc.date.accessioned2019-04-12T14:06:02Z
dc.date.available2019-04-12T14:06:02Z
dc.date.issued2019-04-01
dc.identifier.citationCheale , R A , Geach , J E , Edge , A C , Blain , A W , Chapman , S C , Egami , E , Hogan , M T , Rawle , T D & Webb , T M A 2019 , ' The SCUBA-2 Cluster Snapshot Survey - I. Catalogue of lensed galaxies and submillimetre-bright central galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 484 , no. 2 , pp. 2757-2778 . https://doi.org/10.1093/mnras/stz011
dc.identifier.issn0035-8711
dc.identifier.otherBibtex: urn:7109d13cc9b7bb0bb65896e06f95dade
dc.identifier.urihttp://hdl.handle.net/2299/21258
dc.description© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society
dc.description.abstractThe SCUBA-2 Cluster Snapshot Survey (S2CSS) observed 202 rich clusters of galaxies at 850 μm in relatively poor submillimetre observing conditions (⁠τ225GHz>0.1⁠) with the aim of identifying rare examples of bright (tens of mJy) gravitationally lensed submillimetre galaxies. The S2CSS covered over 0.33 deg2 to an average depth of σ850≈12 mJy beam−1. Here we present a sample of 97 bright 850-μm point sources selected from the S2CSS that are potentially gravitationally lensed, and eight sources for which the strong submillimetre emission is co-located with the central brightest cluster galaxy (BCG). We construct far-infrared spectral energy distributions for those sources with Herschel SPIRE coverage and use these distributions to estimate the redshifts and luminosities of the sources. The bright submillimetre flux density of our sources makes them excellent targets for detailed follow-up work that will allow the detection of spectral features in the submillimetre/millimetre that would otherwise be too faint to detect. Through a stacking analysis, we also investigate the average submillimetre/radio properties of BCGs, determining the average 850-μm flux of BCGs as a function of radio luminosity.en
dc.format.extent22
dc.format.extent27283342
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectgalaxies: active, galaxies: clusters: general, galaxies: evolution, galaxies: high-redshift, cosmology: observations, submillimetre: galaxies
dc.subjectGalaxies: clusters: general
dc.subjectGalaxies: evolution
dc.subjectSubmillimetre: galaxies
dc.subjectCosmology: observations
dc.subjectGalaxies: active
dc.subjectGalaxies: high-redshift
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.titleThe SCUBA-2 Cluster Snapshot Survey - I. Catalogue of lensed galaxies and submillimetre-bright central galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionCentre of Data Innovation Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85063394540&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1093/mnras/stz011
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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