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most citedThe Gemini Deep Deep Survey: III. The abundance of massive galaxies 3-6 billion years after the Big Bang

365 citations · 453 across the 3 of their papers we have counts for

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astro-ph200788 cited

The Gemini Deep Deep Survey: VIII. When Did Early-type Galaxies Form?

Roberto G. Abraham, Preethi Nair, Patrick J. McCarthy +13

We have used the Hubble Space Telescope's Advanced Camera for Surveys (Ford et al. 2003) to measure the cumulative mass density in morphologically-selected early-type galaxies over…

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-ph2004

The mass-metallicity relation at z~0.7

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

The ISM metallicity and the stellar mass are examined in a sample of 66 galaxies at 0.4<z<1, selected from the Gemini Deep Deep Survey (GDDS) and the Canada-France Redshift Survey…

astro-ph2004

Cosmic Star Formation History and its Dependence on Galaxy Stellar Mass

S. Juneau, K. Glazebrook, D. Crampton +11

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). Th…

astro-ph2004

Evolved Galaxies at z > 1.5 from the Gemini Deep Deep Survey: The Formation Epoch of Massive Stellar Systems

Patrick J. McCarthy, Damien Le Borgne, David Crampton +11

We present spectroscopic evidence from the Gemini Deep Deep Survey (GDDS) for a significant population of color-selected red galaxies at 1.3 < z < 2.2 whose integrated light is dom…

astro-ph2004

The Gemini Deep Deep Survey: I. Introduction to the Survey, Catalogs and Composite Spectra

Roberto G. Abraham, Karl Glazebrook, Patrick J. McCarthy +9

The Gemini Deep Deep Survey (GDDS) is an ultra-deep (K<20.6 mag, I<24.5 mag) redshift survey targeting galaxies in the "redshift desert" between 1<z<2. The primary goal of the surv…