H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry
(2015)
Journal Article
Eales, S., Fullard, A., Allen, M., Smith, M., Baldry, I., Bourne, N., Clark, C., Driver, S., Dunne, L., Dye, S., Graham, A. W., Ibar, E., Hopkins, A., Ivison, R., Kelvin, L. S., Maddox, S., Maraston, C., Robotham, A. S., Smith, D., Taylor, E. N., …Serjeant, S. (2015). H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry. Monthly Notices of the Royal Astronomical Society, 452(4), 3489--3507. https://doi.org/10.1093/mnras/stv1300
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.