activity
20042021
most citedBAT AGN Spectroscopic Survey I: Spectral Measurements, Derived Quantities, and AGN Demographics

330 citations · 3.9k across the 50 of their papers we have counts for

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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★ 30 cited

Correlations of the IR Luminosity and Eddington Ratio with a Hard X-ray Selected Sample of AGN

R. F. Mushotzky, L. M. Winter, D. H. McIntosh +1

We use the SWIFT Burst Alert Telescope (BAT) sample of hard x-ray selected active galactic nuclei (AGN) with a median redshift of 0.03 and the 2MASS J and K band photometry to exam…

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★ 106 cited

X-ray properties of an Unbiased Hard X-ray Detected Sample of AGN

Lisa M. Winter, Richard F. Mushotzky, Jack Tueller +1

The SWIFT gamma ray observatory's Burst Alert Telescope (BAT) has detected a sample of active galactic nuclei (AGN) based solely on their hard X-ray flux (14-195 keV). In this pape…

astro-ph2007★ 127 cited

Quasi-Periodic Variability in NGC 5408 X-1

Tod E. Strohmayer, Richard F. Mushotzky, Lisa Winter +3

We report the discovery with XMM-Newton of quasiperiodic variability in the 0.2 - 10 keV X-ray flux from the ultraluminous X-ray source NGC 5408 X-1. The average power spectrum of…