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In Buchner et al. (in prep) a warped disk geometry is studied as an X-ray obscurer of AGN. We irradiate it with a isotropic powerlaw. The model has one geometry parameter, the extent of the warp. Further parameters are: 3) Photon index and energy cut-off of the corona 4) Column density in the line of sight (up to 10^26) 5) Viewing angle. We release XSPEC table spectra.
astronomy, obscured active galactic nuclei, X-ray spectroscopy, Monte Carlo simulation
astronomy, obscured active galactic nuclei, X-ray spectroscopy, Monte Carlo simulation
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