The Evolution of the Global Stellar Mass Density at 0 < z < 3 | Zendy

Mark Dickinson | Zendy; Casey Papovich | Zendy; Henry C. Ferguson | Zendy; Tamás Budavári | Zendy

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The Evolution of the Global Stellar Mass Density at 0 < z < 3

Author(s) -

Mark Dickinson,

Casey Papovich,

Henry C. Ferguson,

Tamás Budavári

Publication year - 2003

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/368111

Subject(s) - physics , astrophysics , stellar mass , galaxy , redshift , star formation , astronomy , luminosity , galaxy formation and evolution , stellar population , extinction (optical mineralogy) , stars , optics

The build-up of stellar mass in galaxies is the consequence of their paststar formation and merging histories. Here we report measurements of rest-frameoptical light and calculations of stellar mass at high redshift based on aninfrared-selected sample of galaxies from the Hubble Deep Field North. Thebright envelope of rest-frame B-band galaxy luminosities is similar from 0>2.Comment: To appear in the Astrophysical Journal. 35 pages, 8 figures, some in colo

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