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

van der Wel, A.; Franx, M.; G. van Dokkum, P.; E. Skelton, R.; G. Momcheva, I.; E. Whitaker, K.; B. Brammer, G.; F. Bell, E.; Rix, H.-W.; Wuyts, S.; C. Ferguson, H.; P. Holden, B.; Barro, G.; M. Koekemoer, A.; Chang, Yu-Yen; J. McGrath, E.; Häussler, B.; Dekel, A.; Behroozi, P.; Fumagalli, M.; Leja, J.; F. Lundgren, B.; V. Maseda, M.; J. Nelson, E.; A. Wake, D.; G. Patel, S.; Labbé, I.; M. Faber, S.; A. Grogin, N.; D. Kocevski, D.

doi:10.1088/0004-637x/788/1/28

Public

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

Shared by NobleBlocks on May 19, 2014 • 12:00 AM UTC

Authors:

A. van der Wel

M. Franx

P. G. van Dokkum

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 g...

Subject

Physics

Astrophysics

Galaxy

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