Cosmic Star Formation History and its Dependence on Galaxy Stellar Mass
We examine the cosmic star formation rate (SFR) and its dependence on galaxy stellar mass over the redshift range 0.8 < z < 2 using data from the Gemini Deep Deep Survey (GDDS). The SFR in the most massive galaxies (M > 10^{10.8} M_sun) was six times higher at z = 2 than it is t...
Auteurs principaux: | Juneau, S, Glazebrook, K, Crampton, D, McCarthy, P, Savaglio, S, Abraham, R, Carlberg, R, Chen, H, Borgne, D, Marzke, R, Roth, K, Jorgensen, I, Hook, I, Murowinski, R |
---|---|
Format: | Journal article |
Publié: |
2005
|
Documents similaires
-
Evolved galaxies at z > 1.5 from the Gemini Deep Deep survey: The formation epoch of massive stellar systems
par: McCarthy, P, et autres
Publié: (2004) -
The Gemini Deep Deep Survey: II. Metals in Star-Forming Galaxies at
Redshift 1.3
par: Savaglio, S, et autres
Publié: (2003) -
A high abundance of massive galaxies 3-6 billion years after the Big Bang.
par: Glazebrook, K, et autres
Publié: (2004) -
The mass-metallicity relation at z ∼ 0.7
par: Savaglio, S, et autres
Publié: (2005) -
The Gemini Deep Deep Survey. I. Introduction to the survey, catalogs, and composite spectra
par: Abraham, R, et autres
Publié: (2004)