3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since \(z=3\)

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 02x10^10 M_sol. The intrinsic scatter is

Saved in:
Bibliographic Details
Published in:arXiv.org 2014-06
Main Authors: van der Wel, A, Franx, M, van Dokkum, P G, Skelton, R E, Momcheva, I G, Whitaker, K E, Brammer, G B, Bell, E F, H -W Rix, Wuyts, S, Ferguson, H C, Holden, B P, Barro, G, Koekemoer, A M, Yu-Yen, Chang, McGrath, E J, Haussler, B, Dekel, A, Behroozi, P, Fumagalli, M, Leja, J, Lundgren, B F, Maseda, M V, Nelson, E J, Wake, D A, Patel, S G, Labbe, I, Faber, S M, Grogin, N A, Kocevski, D D
Format: Article
Language:English
Subjects:
Galactic evolution
Galaxies
Galaxy distribution
Mass distribution
Photometry
Red shift
Size distribution
Star & galaxy formation
Star formation
Stars & galaxies
Stellar mass
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary: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 02x10^10 M_sol. The intrinsic scatter is
ISSN:2331-8422
DOI:10.48550/arxiv.1404.2844