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3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE-MASS DISTRIBUTION SINCE z=3

Abstract:

Spectroscopic+photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging to determine the galaxy size-mass distribution over the redshift range 0 < z < 3. Separating early- and late-type galaxies on the basis of star-formation activity, we confirm that early-type galaxies are on average smaller than late-type galaxies at all redshifts, and we find a significantly different rate of a...

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Publication status:
Published

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Publisher copy:
10.1088/0004-637X/788/1/28

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Publisher:
Institute of Physics Publishing
Journal:
ASTROPHYSICAL JOURNAL
Volume:
788
Issue:
1
Pages:
28-28
Publication date:
2014-06-10
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
URN:
uuid:35dd4975-eaca-4c41-824d-f29d29ee9982
Source identifiers:
470609
Local pid:
pubs:470609

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