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

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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
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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