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20032009
most citedA glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3

625 citations · 1.2k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2009★ 625 cited

A glimpse of the end of the dark ages: the gamma-ray burst of 23 April 2009 at redshift 8.3

N. R. Tanvir, D. B. Fox, A. J. Levan +59

It is thought that the first generations of massive stars in the Universe were an important, and quite possibly dominant, source of the ultra-violet radiation that reionized the hy…

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★ 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-ph2004★ 6 cited

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-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…