The SCUBA-2 Cluster Snapshot Survey – I. Catalogue of lensed galaxies and submillimetre-bright central galaxies
Author
Cheale, Ryan AGeach, James E
Edge, Alastair C
Blain, Andrew W
Chapman, Scott C
Egami, Eiichi
Hogan, Mike T
Rawle, Timothy D
Webb, Tracy M A
Affiliation
Univ Arizona, Steward ObservIssue Date
2019-04-01Keywords
galaxies: activegalaxies: clusters: general
galaxies: evolution
galaxies: high-redshift
cosmology: observations
submillimetre: galaxies
Metadata
Show full item recordPublisher
OXFORD UNIV PRESSCitation
Ryan A Cheale, James E Geach, Alastair C Edge, Andrew W Blain, Scott C Chapman, Eiichi Egami, Mike T Hogan, Timothy D Rawle, Tracy M A Webb, The SCUBA-2 Cluster Snapshot Survey – I. Catalogue of lensed galaxies and submillimetre-bright central galaxies, Monthly Notices of the Royal Astronomical Society, Volume 484, Issue 2, April 2019, Pages 2757–2778, https://doi.org/10.1093/mnras/stz011Rights
© 2019 The Author(s).Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The SCUBA-2 Cluster Snapshot Survey (S2CSS) observed 202 rich clusters of galaxies at 850 mu m in relatively poor submillimetre observing conditions (tau(225) (GHz) > 0.1) with the aim of identifying rare examples of bright (tens of mJy) gravitationally lensed submillimetre galaxies. The S2CSS covered over 0.33 deg(2) to an average depth of sigma(850) approximate to 12 mJy beam(-1). Here we present a sample of 97 bright 850-mu m 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-mu m flux of BCGs as a function of radio luminosity.ISSN
0035-87111365-2966
Version
Final published versionSponsors
Royal Society; Royal Society University Research Fellowship; STFC [ST/P000J41/1]; ERC Advanced Grant [ST/P000J41/1, 321334]; Royal Society/Wolfson Merit Award; Chinese Academy of Sciences [XDB09000000]; Science and Technology Facilities Council of the United KingdomAdditional Links
https://academic.oup.com/mnras/article/484/2/2757/5305294ae974a485f413a2113503eed53cd6c53
10.1093/mnras/stz011
