The Evolution of the Global Stellar Mass Density at 0 < z < 3
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- 10 April 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 587 (1) , 25-40
- https://doi.org/10.1086/368111
Abstract
The build-up of stellar mass in galaxies is the consequence of their past star formation and merging histories. Here we report measurements of rest-frame optical light and calculations of stellar mass at high redshift based on an infrared-selected sample of galaxies from the Hubble Deep Field North. The bright 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 coloKeywords
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