activity
19992006
most citedThe Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging

1.7k citations · 2.4k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph2006★ 11 cited

Hubble Space Telescope Ultraviolet Spectroscopy of Fourteen Low-Redshift Quasars

Rajib Ganguly, Michael S. Brotherton, Nahum Arav +35

We present low-resolution ultraviolet spectra of 14 low redshift (z<0.8) quasars observed with HST/STIS as part of a Snap project to understand the relationship between quasar outf…

astro-ph2005★ 224 cited

AGN Host Galaxies at z~0.4-1.3 : Bulge-dominated and Lacking Merger-AGN Connection

N. A. Grogin, C. J. Conselice, E. Chatzichristou +13

We investigate morphological structure parameters and local environments of distant moderate-luminosity active galactic nucleus (AGN) host galaxies in the overlap between the HST/A…

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…

astro-ph2005

Infrared Properties of AGN in the GOODS Fields: AGN in Stellar Dominated High-z Galaxies

Jeffrey Van Duyne, C. Meg Urry, Eleni Chatzichristou +2

We present analysis of spectral energy distributions (SEDs) from mid-infrared through X-ray of a sample of 420 hard X-ray selected, z-band and Spitzer/IRAC detected active galactic…

astro-ph2004★ 162 cited

Obscured AGN and the X-ray, Optical and Far-Infrared Number Counts of AGN in the GOODS Fields

E. Treister, C. M. Urry, E. Chatzichristou +12

The deep X-ray, optical, and far-infrared fields that constitute GOODS are sensitive to obscured AGN (N_H>10^{22} cm^{-2}) at the quasar epoch (z~2-3), as well as to unobscured AGN…

astro-ph2004

High-redshift QSOs in the GOODS

S. Cristiani, D. M. Alexander, F. Bauer +15

The Great Observatories Origins Deep Survey provides significant constraints on the space density of less luminous QSOs at high redshift, which is particularly important to underst…