346 citations · 1.9k across the 36 of their papers we have counts for
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The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines
I. Strateva, W. N. Brandt, M. Eracleous +2
We summarize the optical, UV, and X-ray properties of double-peaked emitters -- AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We foc…
The X-ray Properties of Early-Type Galaxies in the Extended Chandra Deep Field-South
B. D. Lehmer, W. N. Brandt, D. M. Alexander +8
We investigate the evolution over the last 6.3 Gyr of cosmic time (i.e., since z ~ 0.7) of the average X-ray properties of early-type galaxies within the Extended Chandra Deep Fiel…
Discovery of Variable Iron Fluorescence from Reflection Nebulae in the Galactic Center
M. P. Muno, F. K. Baganoff, W. N. Brandt +2
Based on three years of deep observations of the Galactic center with the Chandra X-ray Observatory, we report the discovery of changes in the intensities and morphologies of two h…
A longer XMM-Newton look at I Zwicky 1: Variability of the X-ray continuum, absorption, and iron Kalpha line
L. C. Gallo, W. N. Brandt, E. Costantini +3
We present the second XMM-Newton observation (85 ks) of the narrow-line Seyfert 1 galaxy (NLS1) I Zw 1 and describe its mean spectral and timing characteristics. On average, I Zw 1…
The X-ray Properties of Active Galactic Nuclei with Double-Peaked Balmer Lines
I. V. Strateva, W. N. Brandt, M. Eracleous +2
Double-peaked Balmer-line profiles originate in the accretion disks of a few percent of optically selected AGN. The reasons behind the strong low-ionization line emission from the…
Chandra Observations of Red Sloan Digital Sky Survey Quasars
Patrick B. Hall, S. C. Gallagher, G. T. Richards +5
We present short \chandra observations of twelve bright (i<18) z_em~1.5 quasars from the Sloan Digital Sky Survey chosen to have significantly redder optical colors than most quasa…