The SCUBA-2 Cosmology Legacy Survey: Demographics of the 450-mu m population

I. G. Roseboom*, J. S. Dunlop, M. Cirasuolo, J. E. Geach, I. Smail, M. Halpern, O. Almaini, V. Arumugam, V. Asboth, R. Auld, A. Blain, M. N. Bremer, J. Bock, R. A. A. Bowler, F. Buitrago, E. Chapin, S. Chapman, A. Chrysostomou, C. Clarke, A. ConleyK. E. K. Coppin, A. L. R. Danielson, D. Farrah, J. Glenn, E. Hatziminaoglou, E. Ibar, R. J. Ivison, T. Jenness, E. Van Kampen, A. Karim, T. Mackenzie, G. Marsden, R. Meijerink, M. J. Michalowski, S. J. Oliver, M. J. Page, E. Pearson, Douglas Scott, J. M. Simpson, D. J. B. Smith, M. Spaans, A. M. Swinbank, M. Symeonidis, T. Targett, E. Valiante, M. Viero, L. Wang, C. J. Willott, M. Zemcov, Paul P. van der Werf

*Corresponding author for this work

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Abstract

We investigate the multiwavelength properties of a sample of 450-μm-selected sources from the SCUBA-2 Cosmology Legacy Survey. A total of 69 sources were identified above 4σ in deep SCUBA-2 450-μm observations overlapping the UDS and COSMOS fields and covering 210 arcmin2 to a typical depth of σ450 = 1.5 mJy. Reliable cross-identifications are found for 58 sources (84 per cent) in Spitzer and Hubble Space Telescope WFC3/IR data. The photometric redshift distribution (dN/dz) of 450-μm-selected sources is presented, showing a broad peak in the redshift range 1 = 1.5 mJy. Reliable cross-identifications are found for 58 sources (84 per cent) in Spitzer and Hubble Space Telescope WFC3/IR data. The photometric redshift distribution (dN/dz) of 450-μm-selected sources is presented, showing a broad peak in the redshift range 1 = 1.5 mJy. Reliable cross-identifications are found for 58 sources (84 per cent) in Spitzer and Hubble Space Telescope WFC3/IR data. The photometric redshift distribution (dN/dz) of 450-μm-selected sources is presented, showing a broad peak in the redshift range 1 = 1.5 mJy. Reliable cross-identifications are found for 58 sources (84 per cent) in Spitzer and Hubble Space Telescope WFC3/IR data. The photometric redshift distribution (dN/dz) of 450-μm-selected sources is presented, showing a broad peak in the redshift range 1 IR> = 1012 ± 0.8 L⊙, , D> = 42 ± 11 K and > = 42 ± 11 K and D> = 1.6 ± 0.5, respectively. The relationship between these SED parameters and the physical properties of galaxies is investigated, revealing correlations between TD and LIR and between βD and both stellar mass and effective radius. The connection between the star formation rate (SFR) and stellar mass is explored, with 24 per cent of 450-μm sources found to be `starbursts', i.e. displaying anomalously high specific SFRs. However, both the number density and observed properties of these `starburst' galaxies are found to be consistent with the population of normal star-forming galaxies.
Original languageEnglish
Pages (from-to)430-448
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume436
Issue number1
DOIs
Publication statusPublished - 21-Nov-2013

Keywords

  • galaxies: evolution
  • galaxies: starburst
  • submillimetre: galaxies
  • STAR-FORMING GALAXIES
  • DEEP FIELD-SOUTH
  • ULTRALUMINOUS INFRARED GALAXIES
  • DEGREE EXTRAGALACTIC SURVEY
  • HIGH-REDSHIFT GALAXIES
  • EQUAL-TO 4
  • SUBMILLIMETER GALAXIES
  • MU-M
  • HERSCHEL-ATLAS
  • NUMBER COUNTS

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