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arXiv · 0704.1253

Compton thick AGN in the Suzaku era

A. Comastri·R. Gilli·C. Vignali·G. Matt·F. Fiore·K. Iwasawa
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Abstract

Suzaku observations of two hard X-ray (> 10 keV) selected nearby Seyfert 2 galaxies are presented. Both sources were clearly detected with the PIN Hard X-ray Detector up to several tens of keV, allowing for a fairly good characterization of the broad band X-ray continuum. Both sources are heavily obscured, one of which (NGC 5728) being Compton thick, while at lower energies the shape and intensity of the scattered/reflected continuum is very different. Strong iron Kalpha lines are detected in both sources. There are also hints for the presence of a broad relativistic iron line in NGC 4992.

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A. Comastri, R. Gilli, C. Vignali, G. Matt, F. Fiore, K. Iwasawa. 2007-04-10. Compton thick AGN in the Suzaku era. https://doi.org/10.1143/ptps.169.274

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