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 language | English |
|---|---|
| Pages (from-to) | 1017-1039 |
| Number of pages | 23 |
| Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
| Volume | 441 |
| Issue number | 2 |
| Early online date | 5 May 2014 |
| DOIs | |
| Publication status | Published - 21 Jun 2014 |
Keywords
- dust, extinction, galaxies: evolution, galaxies: fundamental parameters, galaxies: high-redshift, galaxies: ISM, submillimetre: galaxies