activity
20002009
most citedMid-Infrared Selection of Active Galaxies

936 citations · 1.7k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2009★ 513 cited

Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs

Ryan C. Hickox, Christine Jones, William R. Forman +15

We explore the connection between different classes of active galactic nuclei (AGNs) and the evolution of their host galaxies, by deriving host galaxy properties, clustering, and E…

astro-ph2008★ 24 cited

A Transient Black-Hole Low-Mass X-Ray Binary Candidate in Centaurus A

Gregory R. Sivakoff, Ralph P. Kraft, Andrés Jordán +14

We report the discovery of a bright transient X-ray source, CXOU J132518.2-430304, towards Centaurus A (Cen A) using six new Chandra X-Ray Observatory observations in 2007 March--M…

astro-ph2005★ 10 cited

Intelligent Information Retrieval

Michael J. Kurtz, Guenther Eichhorn, Alberto Accomazzi +3

Since it was first announced at ADASS 2 the Smithsonian/NASA Astrophysics System Abstract Service (ADS) has played a central role in the information seeking behavior of astronomers…

astro-ph2004★ 936 cited

Mid-Infrared Selection of Active Galaxies

Daniel Stern, Peter Eisenhardt, Varoujan Gorjian +12

Mid-infrared photometry provides a robust technique for identifying active galaxies. While the ultraviolet to mid-infrared continuum of normal galaxies is dominated by the composit…

astro-ph2002★ 140 cited

New Constraints on Neutron Star Cooling from Chandra Observations of 3C58

Patrick Slane, David J. Helfand, Stephen S. Murray

3C58 is a young Crab-like supernova remnant. Historical evidence strongly suggests an association of the remnant with supernova SN 1181, which would make 3C58 younger than the Crab…

astro-ph2001★ 65 cited

Bright X-Ray Sources in M31 Globular Clusters

R. Di Stefano, A. K. H. Kong, M. R. Garcia +4

We have conducted Chandra observations of ~2560 square arcmin (~131 kpc^2) of of M31, and find that the most luminous X-ray sources in our fields are in globular clusters (GCs). Of…