Journal Article

The relationship between star formation rates, local density and stellar mass up to <i>z</i> ∼ 3 in the GOODS NICMOS Survey

R. Grützbauch, C. J. Conselice, A. E. Bauer, A. F. L. Bluck, R. W. Chuter, F. Buitrago, A. Mortlock, T. Weinzirl and S. Jogee

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 418, issue 2, pages 938-948
Published in print December 2011 | ISSN: 0035-8711
Published online November 2011 | e-ISSN: 1365-2966 | DOI:
The relationship between star formation rates, local density and stellar mass up to z ∼ 3 in the GOODS NICMOS Survey

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics


Show Summary Details


We investigate the relation between star formation rates and local galaxy environment for a stellar-mass-selected galaxy sample in the redshift range 1.5 ≤z≤ 3. We use near-infrared imaging from an extremely deep Hubble Space Telescope survey, the GOODS NICMOS Survey (GNS), to measure local galaxy densities based on the nearest neighbour approach, while star formation rates are estimated from rest-frame ultraviolet fluxes. Due to our imaging depth, we can examine galaxies down to a colour-independent stellar mass completeness limit of log M*= 9.5 M at z∼ 3. We find a strong dependence of star formation activity on galaxy stellar mass over the whole redshift range, which does not depend on local environment. The average star formation rates are largely independent of local environment, apart from those in the highest relative overdensities. Galaxies in overdensities of a factor of >5 have on average lower star formation rates by a factor of 2–3, but only up to redshifts of z∼ 2. We do not see any evidence for active galactic nucleus activity influencing these relations. We also investigate the influence of the very local environment on star formation activity by counting neighbours within 30 kpc radius. This shows that galaxies with two or more close neighbours have on average significantly lower star formation rates as well as lower specific star formation rates up to z∼ 2.5. We suggest that this might be due to star formation quenching induced by galaxy merging processes.

Keywords: galaxies: evolution; galaxies: high-redshift

Journal Article.  8791 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.