H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry

H-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetry

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 early-type galaxies (ETGs; Sérsic n > 2.5) whil...

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Bibliographic Details
Main Authors: Eales, Stephen, Fullard, Andrew, Allen, Matthew, Smith, M.W.L., Baldry, Ivan, Bourne, Nathan, Clark, C.J.R., Driver, Simon, Dunne, Loretta, Dye, S., Graham, Alister W., Ibar, Edo, Hopkins, Andrew, Ivison, Rob, Kelvin, Lee S., Maddox, Steve, Maraston, Claudia, Robotham, Aaron S.G., Smith, Dan, Taylor, Edward N., Valiante, Elisabetta, Werf, Paul van der, Baes, Maarten, Brough, Sarah, Clements, David, Cooray, Asantha, Gomez, Haley, Loveday, Jon, Phillipps, Steven, Scott, Douglas, Serjeant, Steve
Format: Article
Published: Oxford University Press 2015
Subjects:
galaxies: bulges
galaxies: evolution
galaxies: star formation
Online Access:https://eprints.nottingham.ac.uk/42390/

Internet

https://eprints.nottingham.ac.uk/42390/

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