The redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDS

In this paper we present a detailed study of the structures and morphologies of a sample of 1188 massive galaxies with M * ≥ 1010 M between redshifts z = 1 and 3 within the Ultra Deep Survey (UDS) region of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) field. Using thi...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-08, Vol.433 (2), p.1185-1201
Hauptverfasser:	Mortlock, Alice, Conselice, Christopher J., Hartley, William G., Ownsworth, Jamie R., Lani, Caterina, Bluck, Asa F. L., Almaini, Omar, Duncan, Kenneth, Wel, Arjen van der, Koekemoer, Anton M., Dekel, Avishai, Davé, Romeel, Ferguson, Harry C., de Mello, Duilia F., Newman, Jeffrey A., Faber, Sandra M., Grogin, Norman A., Kocevski, Dale D., Lai, Kamson
Format:	Artikel
Sprache:	eng
Schlagworte:	Morphology Red shift Simulation Stars & galaxies
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