Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts

  • K. Rowlands
  • , L. Dunne
  • , S. Dye
  • , A. Aragón-Salamanca
  • , S. Maddox
  • , E. da Cunha
  • , Daniel Smith
  • , N. Bourne
  • , S. Eales
  • , H.L. Gomez
  • , I. Smail
  • , M. Alpaslan
  • , C.J.R. Clark
  • , S. Driver
  • , E. Ibar
  • , Rob J. Ivison
  • , A. Robotham
  • , M.W.L. Smith
  • , E. Valiante

Research output: Contribution to journalArticlepeer-review

62 Citations (Scopus)
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Abstract

We present a comparison of the physical properties of a rest-frame 250-μm-selected sample of massive, dusty galaxies from 0 < z < 5.3. Our sample comprises 29 high-redshift submillimetre galaxies (SMGs) from the literature and 843 dusty galaxies at z < 0.5 from the Herschel-Astrophysical TeraHertz Large Area Survey (H-ATLAS), selected to have a similar stellar mass to the SMGs
Original languageEnglish
Pages (from-to)1017-1039
Number of pages23
JournalMonthly Notices of the Royal Astronomical Society (MNRAS)
Volume441
Issue number2
Early online date5 May 2014
DOIs
Publication statusPublished - 21 Jun 2014

Keywords

  • dust, extinction, galaxies: evolution, galaxies: fundamental parameters, galaxies: high-redshift, galaxies: ISM, submillimetre: galaxies

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