activity
19952019
most citedThe Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging

1.7k citations · 6.5k across the 46 of their papers we have counts for

collaborators
Showing astro-phShow all

31 papers · 1 filter

astro-ph2008★ 21 cited

A Study of Quasar Proximity in O VI Absorbers at z=2-3

Andrew J. Fox, Jacqueline Bergeron, Patrick Petitjean

(Abridged) With the goal of investigating the nature of OVI absorbers at high redshifts, we study the effects of proximity to the background quasar. In a sample of sixteen quasars…

astro-ph2007★ 262 cited

Four quasars above redshift 6 discovered by the Canada-France High-z Quasar Survey

Chris J. Willott, Philippe Delorme, Alain Omont +15

The Canada-France High-z Quasar Survey (CFHQS) is an optical survey designed to locate quasars during the epoch of reionization. In this paper we present the discovery of the first…

astro-ph2005★ 65 cited

Where are the missing cosmic metals ?

A. Ferrara, E. Scannapieco, J. Bergeron

The majority of the heavy elements produced by stars 2 billion years after the Big Bang (redshift z~3) are presently undetected at those epochs. We propose a solution to this cosmi…

astro-ph2005★ 3 cited

Highly ionized absorbers at high redshift

Jacqueline Bergeron, Stéphane Herbert-Fort

We investigate the existence of a metal-rich OVI population in 10 high spectral resolution quasar spectra and define observational criteria for this class of absorbers. The low tem…

astro-ph2005★ 1 cited

The sub-DLA toward HE0001-2340: galaxy formation at z=2

P. Richter, C. Ledoux, P. Petitjean +1

We present a detailed analysis of chemical abundances in a sub-damped Ly alpha absorber (sub-DLA) at z=2.187 towards the quasar HE0001-2340 (z_em=2.28) using VLT/UVES data. This su…

astro-ph2005

Infrared Number Counts of AGN in the GOODS Fields

E. Treister, C. Megan Urry, the GOODS AGN Team

Using the known numbers and evolution of unobscured AGN, and assuming that there is a large number of corresponding obscured AGN -- as expected if AGN unification is correct -- we…