Unified Clumpy Agn Torus Model And X-Ray Spectrum

In Buchner et al. (in prep) develop a geometry for the X-ray obscurer of AGN. Its cloud population is consistent with existing CLUMPY (Nenkova+02) models. However, we find that a inner torus ring component is required. Our model has two geometry parameter:<br> 1) The opening of the torus, or the vertical extent of the clouds (sigma)<br> 2) The covering of the inner Compton-thick wall.<br> Further parameters are:<br> 3) Photon index and energy cut-off of the corona<br> 4) Column density in the line of sight (up to 10^26)<br> 5) Viewing angle. We release XSPEC table spectra.