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

  • Dickinson M
  • Papovich C
  • Ferguson H
  • et al.
The Astrophysical Journal (2003) 587(1) 25-40
DOI: 10.1086/368111
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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.

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APA

Dickinson, M., Papovich, C., Ferguson, H. C., & Budavari, T. (2003). The Evolution of the Global Stellar Mass Density at 0 < z < 3. The Astrophysical Journal, 587(1), 25–40. https://doi.org/10.1086/368111

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