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19932024
most citedOn characterising the variability properties of X-ray light curves from active galaxies

1.2k citations · 6.4k across the 65 of their papers we have counts for

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astro-ph2004★ 118 cited

An Expanded RXTE Survey of X-ray Variability in Seyfert 1 Galaxies

Alex Markowitz, Rick Edelson

The first seven years of RXTE monitoring of Seyfert 1 active galactic nuclei have been systematically analyzed to yield five homogeneous samples of 2-12 keV light curves, probing h…

astro-ph2004★ 32 cited

Chandra observations of five X-ray transient galactic nuclei

S. Vaughan, R. Edelson, R. S. Warwick

We report on exploratory Chandra observations of five galactic nuclei that were found to be X-ray bright during the ROSAT all-sky survey (with L_X > 10^43 erg s^-1) but subsequentl…

astro-ph2003★ 132 cited

Long-Term X-ray Spectral Variability in Seyfert 1 Galaxies

A. Markowitz, R. Edelson, S. Vaughan

Direct time-resolved spectral fitting has been performed on continuous RXTE monitoring of seven Seyfert 1 galaxies in order to study their broadband spectral variability and Fe K a…

astro-ph2003★ 1.2k cited

On characterising the variability properties of X-ray light curves from active galaxies

S. Vaughan, R. Edelson, R. S. Warwick +1

We review some practical aspects of measuring the amplitude of variability in `red noise' light curves typical of those from Active Galactic Nuclei (AGN). The quantities commonly u…

astro-ph2003★ 40 cited

Contrasting the UV and X-ray O VI Column Density Inferred for the Outflow in NGC 5548

Nahum Arav, Jelle Kaastra, Katrien Steenbrugge +4

We compare X-ray and UV spectroscopic observations of NGC 5548. Both data sets show O VI absorption troughs associated with the AGN outflow from this galaxy. We find that the robus…

astro-ph2003★ 125 cited

XMM-NEWTON High Resolution Spectroscopy of NGC 5548

K. C. Steenbrugge, J. S. Kaastra, C. P. de Vries +1

We analyze a 137 ks exposure X-ray spectrum of the Seyfert 1 galaxy NGC 5548 obtained with the XMM-Newton Reflection Grating Spectrometer. Due to the long exposure time, the spectr…