485 citations · 786 across the 10 of their papers we have counts for
10 papers
Exploring the z=3-4 massive galaxy population with ZFOURGE: the prevalence of dusty and quiescent galaxies
Lee R. Spitler, Caroline M. S. Straatman, Ivo Labbe +17
Our understanding of the redshift galaxy population relies largely on samples selected using the popular "dropout" technique, typically consisting of UV-bright galaxies with…
The slowly evolving role of environment in a spectroscopic survey of star formation in Mstar > 5E8 Msun galaxies since z=1
Chad R. Greene, David G. Gilbank, Michael L. Balogh +6
We present a deep [OII] emission line survey of faint galaxies (22.5<KAB<24) in the Chandra Deep Field South and the FIRES field. With these data we measure the star formation rate…
A spectroscopic measurement of galaxy formation timescales with ROLES
David G. Gilbank, Richard G. Bower, Karl Glazebrook +7
We present measurements of the specific star-formation rate (SSFR)-stellar mass relation for star-forming galaxies. Our deep spectroscopic samples are based on the Redshift One LDS…
Dependence of Star Formation Activity On Stellar Mass and Environment From the Redshift One LDSS-3 Emission Line Survey (ROLES)
I. H. Li, Karl Glazebrook, David Gilbank +6
Using the sample from the \it Redshift One LDSS3 Emission line Survey \rm (ROLES), we probe the dependence of star formation rate (SFR) and specific star formation rate (sSFR) as a…
The Redshift One LDSS-3 Emission line Survey (ROLES) II: Survey method and z~1 mass-dependent star-formation rate density
David G. Gilbank, Michael L. Balogh, Karl Glazebrook +6
Motivated by suggestions of 'cosmic downsizing', in which the dominant contribution to the cosmic star formation rate density (SFRD) proceeds from higher to lower mass galaxies wit…
A spectroscopic measure of the star-formation rate density in dwarf galaxies at z~1
G. T. Davies, David Gilbank, Karl Glazebrook +7
We use a K-selected (22.5 < K_AB < 24.0) sample of dwarf galaxies (8.4 < log(M*/Msun) < 10) at 0.89<z<1.15 in the Chandra Deep Field South (CDFS) to measure their contribution to t…