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19982008
most citedThe Gemini Deep Deep Survey: III. The abundance of massive galaxies 3-6 billion years after the Big Bang

365 citations · 366 across the 3 of their papers we have counts for

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Showing 2004 · astro-phShow all

6 papers · 2 filters

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

Near-Infrared Properties of Faint X-rays Sources from NICMOS Imaging in the Chandra Deep Fields

James W. Colbert, Harry Teplitz, Lin Yan +2

We measure the near-infrared properties of 42 X-ray detected sources from the Chandra Deep Fields North and South, the majority of which lie within the NICMOS Hubble Deep Field Nor…

astro-ph2004

Optical and Infrared Photometry of the Type Ia Supernovae 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, and 2002bo

Kevin Krisciunas, Nicholas B. Suntzeff, Mark M. Phillips +28

We present optical and/or infrared photometry of the Type Ia supernovae SN 1991T, SN 1991bg, SN 1999ek, SN 2001bt, SN 2001cn, SN 2001cz, and SN 2002bo. All but one of these superno…

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…

astro-ph2004365 cited

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

Karl Glazebrook, Roberto Abraham, Patrick McCarthy +9

Hierarchical galaxy formation is the model whereby massive galaxies form from an assembly of smaller units. The most massive objects therefore form last. The model succeeds in desc…