Research output: Contribution to journal › Article › peer-review
- 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
Notes
Date of Acceptance: 09/03/2014
ID: 8295498