3D-HST+candels: the evolution of the galaxy size-mass distribution since z = 3

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.; Rix, H.-W.; Wuyts, S.; Ferguson, H. C.; Holden, B. P.; Barro, G.; Koekemoer, A. M.; Chang, Yu-Yen; McGrath, E. J.; Häussler, B.; Dekel, A.; Behroozi, P.; Fumagalli, M.; Leja, J.; Lundgren, B. F.; Maseda, M. V.; Nelson, E. J.; Wake, D. A.; Patel, S. G.; Labbé, I.; Faber, S. M.; Grogin, N. A.; Kocevski, D. D.

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

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3D-HST+candels: the evolution of the galaxy size-mass distribution since z = 3

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Wuyts, S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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van der Wel, A., Franx, M., van Dokkum, P. G., Skelton, R. E., Momcheva, I. G., Whitaker, K. E., et al. (2014). 3D-HST+candels: the evolution of the galaxy size-mass distribution since z = 3. The Astrophysical Journal, 788(1): 28. doi:10.1088/0004-637X/788/1/28.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0027-770B-1

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