A Systematic Study of the Global Stellar Mass Density at 0.5<z<6

Details A Systematic Study of the Global Stellar Mass Density at 0.5<z<6 A Systematic Study of the Global Stellar Mass Density at 0.5<z<6

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40836y&link_type=abstract

Spitzer Proposal ID #40836

Computer Science

Scientific paper

Global stellar mass density is one of the two basic quantities that describe the global star formation activities in the universe, and the study of its evolution is of fundamental importance in understanding the mass assembly history of galaxies. However, the measurement of this quantity remains scarce, largely due to the lack of deep, wide-field IR imaging data that are critical in estimating the stellar masses of galaxies. Spitzer/IRAC offers an unprecedented opportunity in advancing this study. The investigator proposes to carry out a systematic study of the stellar mass density at 0.5

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