Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(452), p. 3489-3507
Links
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- ORCID
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- ORCID
- Oxford University Press (OUP)
- [researchonline.ljmu.ac.uk]
- [research-information.bristol.ac.uk] | PDF
- [biblio.ugent.be] | PDF
- [uhra.herts.ac.uk] | PDF
- [research-repository.st-andrews.ac.uk] | PDF
- [openaccess.leidenuniv.nl] | PDF
- [sro.sussex.ac.uk] | PDF
- [spiral.imperial.ac.uk] | PDF
- [researchonline.ljmu.ac.uk] | PDF
- [orca.cf.ac.uk] | PDF
- [eprints.nottingham.ac.uk] | PDF
- [arxiv.org] | PDF
- [www.researchgate.net] | PDF
- [arxiv.org] | PDF
- [researchonline.ljmu.ac.uk] | PDF
- [biblio.ugent.be] | PDF
- [research-information.bristol.ac.uk] | PDF
Tools
H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry
Journal article published in 2015 by
Stephen Eales,
Andrew Fullard,
Matthew Allen,
Mwl W. L. Smith,
Ik Baldry,
Nathan Bourne,
Cjr J. R. Clark,
Simon Driver,
Loretta Dunne,
Simon Dye 
,
Aw Graham ,
Edo Ibar,
Andrew Hopkins,
Rob Ivison,
Ls Kelvin
and other authors.
,
Aw Graham ,
Edo Ibar,
Andrew Hopkins,
Rob Ivison,
Ls Kelvin
and other authors.
This paper is available in a repository.
Full text: Download
Data provided by 
Abstract
Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar masses, 51% of the stellar mass-density in the local Universe is in early-type galaxies (ETGs: Sersic n > 2.5) while 89% of the rate of production of stellar mass-density is occurring in late-type galaxies (LTGs: Sersic n