Aaron Wilkinson
The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field
Wilkinson, Aaron; Almaini, Omar; Chen, Chian Chou; Smail, Ian; Arumugam, Vinodiran; Blain, Andrew; Chapin, Edward L.; Chapman, Scott C.; Conselice, Christopher J.; Cowley, William I.; Dunlop, James S.; Farrah, Duncan; Geach, James; Hartley, William G.; Ivison, Rob J.; Maltby, David T.; Micha?owski, Micha? J.; Mortlock, Alice; Scott, Douglas; Simpson, Chris; Simpson, James M.; van der Werf, Paul; Wild, Vivienne
Authors
OMAR ALMAINI omar.almaini@nottingham.ac.uk
Professor of Astrophysics
Chian Chou Chen
Ian Smail
Vinodiran Arumugam
Andrew Blain
Edward L. Chapin
Scott C. Chapman
Christopher J. Conselice
William I. Cowley
James S. Dunlop
Duncan Farrah
James Geach
William G. Hartley
Rob J. Ivison
David T. Maltby
Micha? J. Micha?owski
Alice Mortlock
Douglas Scott
Chris Simpson
James M. Simpson
Paul van der Werf
Vivienne Wild
Abstract
© 2016 The Authors. Submillimetre galaxies (SMGs) are among the most luminous dusty galaxies in the Universe, but their true nature remains unclear; are SMGs the progenitors of the massive elliptical galaxies we see in the local Universe, or are they just a short-lived phase among more typical star-forming galaxies? To explore this problem further, we investigate the clustering of SMGs identified in the SCUBA-2 Cosmology Legacy Survey. We use a catalogue of submillimetre (850 μm) source identifications derived using a combination of radio counterparts and colour/infrared selection to analyse a sample of 610 SMG counterparts in the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Survey (UKIDSS) Ultra Deep Survey (UDS), making this the largest high-redshift sample of these galaxies to date. Using angular cross-correlation techniques, we estimate the halo masses for this large sample of SMGs and compare them with passive and star-forming galaxies selected in the same field. We find that SMGs, on average, occupy high-mass dark matter haloes (Mhalo > 1013 M⊙) at redshifts z > 2.5, consistent with being the progenitors of massive quiescent galaxies in present-day galaxy clusters. We also find evidence of downsizing, in which SMG activity shifts to lower mass haloes at lower redshifts. In terms of their clustering and halo masses, SMGs appear to be consistent with other star-forming galaxies at a given redshift.
Citation
Wilkinson, A., Almaini, O., Chen, C. C., Smail, I., Arumugam, V., Blain, A., …Wild, V. (2017). The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field. Monthly Notices of the Royal Astronomical Society, 464(2), 1380-1392. https://doi.org/10.1093/mnras/stw2405
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 21, 2016 |
Online Publication Date | Sep 22, 2016 |
Publication Date | Jan 1, 2017 |
Deposit Date | Jan 13, 2017 |
Publicly Available Date | Jan 13, 2017 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 464 |
Issue | 2 |
Pages | 1380-1392 |
DOI | https://doi.org/10.1093/mnras/stw2405 |
Keywords | galaxies: evolution ; galaxies: formation ; galaxies: high-redshift ; galaxies: starburst ; large-scale structure of Universe. |
Public URL | https://nottingham-repository.worktribe.com/output/830980 |
Publisher URL | https://academic.oup.com/mnras/article/464/2/1380/2282841/The-SCUBA-2-Cosmology-Legacy-Survey-the-clustering |
Contract Date | Jan 13, 2017 |
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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
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