Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(421), p. 3027-3059
DOI: 10.1111/j.1365-2966.2012.20528.x
Full text: Download
We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the submillimetre properties of optically selected galaxies. Using similar to 80 000 r-band selected galaxies from 126 deg2 of the GAMA survey, we stack into submillimetre imaging at 250, 350 and 500 mu m to gain unprecedented statistics on the dust emission from galaxies at z