University of Hertfordshire

From the same journal

From the same journal

By the same authors

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

Research output: Contribution to journalArticlepeer-review

Documents

  • 907018

    Accepted author manuscript, 3.38 MB, PDF document

  • 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
View graph of relations
Original languageEnglish
Pages (from-to)1017-1039
Number of pages23
JournalMonthly Notices of the Royal Astronomical Society
Volume441
Issue2
Early online date5 May 2014
DOIs
Publication statusPublished - 21 Jun 2014

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

Notes

Date of Acceptance: 09/03/2014

ID: 8295498