H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry
(2015)
Journal Article
Using results from the Herschel Astrophysical Terrahertz Large-Area Survey (H-ATLAS) and the Galaxy and Mass Assembly (GAMA) project, we show that, for galaxy masses above ≃ 108 M⊙, 51 per cent of the stellar mass-density in the local Universe is in... Read More about H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry.