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19952009
most citedThe Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation

485 citations · 923 across the 12 of their papers we have counts for

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11 papers · 1 filter

astro-ph2008

A New Window of Exploration in the Mass Spectrum: Strong Lensing by Galaxy Groups in the SL2S

M. Limousin, R. Cabanac, R. Gavazzi +21

The existence of strong lensing systems with Einstein radii (Re) covering the full mass spectrum, from ~1-2" (produced by galaxy scale dark matter haloes) to >10" (produced by gala…

astro-ph2007★ 23 cited

A Compact Cluster of Massive Red Galaxies at a Redshift of 1.51

P. J. McCarthy, H. Yan, R. G. Abraham +15

We describe a compact cluster of massive red galaxies at z=1.51 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep imaging with the Near Infrared Camera and Multi…

astro-ph2006

When do early-type galaxies form?

Roberto G. Abraham, Patrick J. McCarthy, Erin Mentuch +13

We have used the Hubble Space Telescope's Advanced Camera for Surveys to measure the mass density function of morphologically selected early-type galaxies in the Gemini Deep Deep S…

astro-ph2005

GDDS Highlights: Galaxy Evolution Revealed

David Crampton, the GDDS Team

The Gemini Deep Deep Survey, GDDS, produced several significant results relating to the evolution of galaxies. All of these results are consistent with the "downsizing" concept of…

astro-ph2005★ 485 cited

The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation

S. Savaglio, K. Glazebrook, D. Le Borgne +10

We have investigated the mass-metallicity (M-Z) relation using galaxies at 0.4<z<1.0 from the Gemini Deep Deep Survey and Canada-France Redshift Survey. Deep K and z' band photomet…

astro-ph2003★ 52 cited

The Gemini Deep Deep Survey: II. Metals in Star-Forming Galaxies at Redshift 1.3<z<2

S. Savaglio, K. Glazebrook, R. G. Abraham +9

The goal of the Gemini Deep Deep Survey (GDDS) is to study an unbiased sample of K<20.6 galaxies in the redshift range 0.8<z<2.0. Here we determine the statistical properties of th…