X-Ray Variability of Active Galactic Nuclei in the Lockman Hole

Details X-Ray Variability of Active Galactic Nuclei in the Lockman Hole X-Ray Variability of Active Galactic Nuclei in the Lockman Hole

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.0207c&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #02.07; Bulletin of the American Astronomical Society, Vol. 32, p.1183

Astronomy and Astrophysics

Astronomy

Scientific paper

The Lockman Hole (a high-latitude region of extremely low Galactic H I column density) has been a favorite target for deep studies of the cosmic soft X-ray background for 15 years. Hundreds of kiloseconds of effective exposure have been collected by ROSAT over a time span of years. Here, we present an analysis of the X-ray variability properties of the many bright AGN in this field on time scales ranging from hours to years, based on an analysis of archival ROSAT data. These AGN have a typical redshift of z ~ 1.

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