activity
20012007
most citedObscured AGN and the X-ray, Optical and Far-Infrared Number Counts of AGN in the GOODS Fields

162 citations · 369 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2007★ 106 cited

Halo Star Streams in the Solar Neighborhood

Amanda A. Kepley, Heather L. Morrison, Amina Helmi +6

We have assembled a sample of halo stars in the solar neighborhood to look for halo substructure in velocity and angular momentum space. Our sample includes red giants, RR Lyrae, a…

astro-ph2006★ 101 cited

Shedding New Light on the 3C 273 Jet with the Spitzer Space Telescope

Y. Uchiyama, C. M. Urry, C. C. Cheung +7

We have performed infrared imaging of the jet of the quasar 3C 273 at wavelengths 3.6 and 5.8 microns with the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. When com…

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

Obscured AGN in Multiwavelength Surveys

Ezequiel Treister, C. M. Urry, Jeff Van Duyne +1

Using a simple unification model for AGN, with a fixed ratio of obscured to unobscured AGN of 3:1, we explain the X-ray, optical and infrared properties of the X-ray sources in the…

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…