Specific Star Formation Rates to Redshift 1.5
Abstract
We present a study to determine how star formation contributes to galaxy growth since z=1.5 over five decades in galaxy stellar mass. We investigate the specific star formation rate (SSFR; star formation rate [SFR] per unit galaxy stellar mass) as a function of galaxy stellar mass and redshift. A sample of 175 K-band-selected galaxies from the MUnich Near-Infrared Cluster Survey spectroscopic data set provides intermediate- to high-mass galaxies (mostly M*>=1010 Msolar) to z=1. The FORS Deep Field provides 168 low-mass galaxies (mostly M*<=1010 Msolar) to z=1.5. We use a Sloan Digital Sky Survey galaxy sample to test the compatibility of our results with data drawn from a larger volume. We find that at all redshifts, the SSFR decreases with increasing galaxy stellar mass, suggesting that star formation contributes more to the growth of low-mass galaxies than to the growth of high-mass galaxies and that high-mass galaxies formed the bulk of their stellar content before z=1. At each epoch, we find a ridge in SSFR versus stellar mass that is parallel to lines of constant SFR and evolves independently of galaxy stellar mass to a particular turnover mass. Galaxies above this turnover mass show a sharp decrease in the SFR compared to the average at each epoch, and the turnover mass increases with redshift. The SFR along the SSFR ridge decreases by roughly a factor of 10, from 10 Msolar yr-1 at z=1.5 to 1 Msolar yr-1 at z=0. High-mass galaxies could sustain the observed rates of star formation over the 10 Gyr observed, but low-mass galaxies likely undergo episodic starbursts.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 2005
- DOI:
- 10.1086/429289
- arXiv:
- arXiv:astro-ph/0412358
- Bibcode:
- 2005ApJ...621L..89B
- Keywords:
-
- Galaxies: Evolution;
- Galaxies: Stellar Content;
- Surveys;
- Astrophysics
- E-Print:
- 4 pages, 2 figures, matches ApJL accepted version