activity
19952026
most citedThe Nature of Accreting Black Holes in Nearby Galaxy Nuclei

671 citations · 11.7k across the 116 of their papers we have counts for

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astro-ph2008★ 57 cited

The OPTX Project I: The Flux and Redshift Catalogs for the CLANS, CLASXS, and CDF-N fields

L. Trouille, A. J. Barger, L. L. Cowie +2

We present the redshift catalogs for the X-ray sources detected in the Chandra Deep Field North (CDF-N), the Chandra Large Area Synoptic X-ray Survey (CLASXS), and the Chandra Lock…

astro-ph2008★ 71 cited

Constraining the AGN Contribution in a Multiwavelength Study of Seyfert Galaxies

M. Meléndez, S. B. Kraemer, H. R. Schmitt +4

We have studied the relationship between the high- and low-ionization [O IV] lambda 25.89 micron, [Ne III] lambda 15.56 micron and [Ne II] lambda 12.81 micron emission lines with t…

astro-ph2008★ 265 cited

X-ray Spectral Properties of the BAT AGN Sample

L. M. Winter, R. Mushotzky, C. S. Reynolds +1

The 9-month Swift Burst Alert Telescope (BAT) catalog provides the first unbiased (log N_H < 24) look at local (<z> = 0.03) AGN. In this paper, we present the collected X-ray prope…

astro-ph2008★ 147 cited

New Indicators for AGN Power: The Correlation Between [O IV] lambda 25.89 micron and Hard X-ray Luminosity for Nearby Seyfert Galaxies

M. Meléndez, S. B. Kraemer, B. K Armentrout +7

We have studied the relationship between the [O IV] lambda 25.89 micron emission line luminosities, obtained from Spitzer spectra, the X-ray continua in the 2-10 keV band, primaril…

astro-ph2007★ 301 cited

Swift BAT Survey of AGN

J. Tueller, R. F. Mushotzky, S. Barthelmy +5

We present the results of the analysis of the first 9 months of data of the Swift BAT survey of AGN in the 14-195 keV band. Using archival X-ray data or follow-up Swift XRT observa…

astro-ph2007★ 27 cited

The Suzaku Observation of NGC 3516: Complex Absorption and the Broad and Narrow Fe K Lines

A. Markowitz, J. N. Reeves, G. Miniutti +10

We present results from a 150 ksec Suzaku observation of the Seyfert 1.5 NGC 3516 in October 2005. The source was in a relatively highly absorbed state. Our best-fit model is consi…