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

Mark Dickinson·Casey Papovich·Henry C. Ferguson·Tamas Budavari
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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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Mark Dickinson, Casey Papovich, Henry C. Ferguson, Tamas Budavari. 2002-12-10. The Evolution of the Global Stellar Mass Density at 0 < z < 3. https://doi.org/10.1086/368111

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