The Evolution of the Global Stellar Mass Density at 0 < z < 3
Preprint
- 10 December 2002
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 02.Keywords
All Related Versions
- Version 1, 2002-12-10, ArXiv
- Published version: The Astrophysical Journal, 587 (1), 25.
This publication has 0 references indexed in Scilit: