The Evolution of the global stellar mass density at 0 < z < 3
Dec, 200235 pages
Published in:
- Astrophys.J. 587 (2003) 25-40
e-Print:
- astro-ph/0212242 [astro-ph]
DOI:
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Abstract: (arXiv)
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 0References(0)
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