Accretion Disk Models in the Kerr geometry (Siemiginowska et al. 1995) The files in this directory contain predicted spectra emitted by an accretion disk surrounding supermassive black hole (section 4.1). Effects of electron scattering in the atmosphere of the disk are taken into account (local modified blackbody and Comptonization). Also bound-free opacities are included following Maraschi & Molendi (1990). The files are: Filename Model Parameters ----------------------------------------------------------------------------- Log Black Hole Mass Accretion Rate Inclination Angle (in solar mass) (in Eddington) (cos theta) k7_01a.dat 7.0 0.1 0.1 k7_01b.dat 7.0 0.1 0.25 k7_01c.dat 7.0 0.1 0.5 k7_01d.dat 7.0 0.1 0.75 k7_01e.dat 7.0 0.1 1.0 k7_03a.dat 7.0 0.3 0.1 k7_03b.dat 7.0 0.3 0.25 k7_03c.dat 7.0 0.3 0.5 k7_03d.dat 7.0 0.3 0.75 k7_03e.dat 7.0 0.3 1.0 k7_08a.dat 7.0 0.8 0.1 k7_08b.dat 7.0 0.8 0.25 k7_08c.dat 7.0 0.8 0.5 k7_08d.dat 7.0 0.8 0.75 k7_08e.dat 7.0 0.8 1.0 k8_01a.dat 8.0 0.1 0.1 k8_01b.dat 8.0 0.1 0.25 k8_01c.dat 8.0 0.1 0.5 k8_01d.dat 8.0 0.1 0.75 k8_01e.dat 8.0 0.1 1.0 k8_03a.dat 8.0 0.3 0.1 k8_03b.dat 8.0 0.3 0.25 k8_03c.dat 8.0 0.3 0.5 k8_03d.dat 8.0 0.3 0.75 k8_03e.dat 8.0 0.3 1.0 k8_08a.dat 8.0 0.8 0.1 k8_08b.dat 8.0 0.8 0.25 k8_08c.dat 8.0 0.8 0.5 k8_08d.dat 8.0 0.8 0.75 k8_08e.dat 8.0 0.8 1.0 k9_01a.dat 9.0 0.1 0.1 k9_01b.dat 9.0 0.1 0.25 k9_01c.dat 9.0 0.1 0.5 k9_01d.dat 9.0 0.1 0.75 k9_01e.dat 9.0 0.1 1.0 k9_03a.dat 9.0 0.3 0.1 k9_03b.dat 9.0 0.3 0.25 k9_03c.dat 9.0 0.3 0.5 k9_03d.dat 9.0 0.3 0.75 k9_03e.dat 9.0 0.3 1.0 k9_08a.dat 9.0 0.8 0.1 k9_08b.dat 9.0 0.8 0.25 k9_08c.dat 9.0 0.8 0.5 k9_08d.dat 9.0 0.8 0.75 k9_08e.dat 9.0 0.8 1.0 k10_01a.dat 10.0 0.1 0.1 k10_01b.dat 10.0 0.1 0.25 k10_01c.dat 10.0 0.1 0.5 k10_01d.dat 10.0 0.1 0.75 k10_01e.dat 10.0 0.1 1.0 k10_03a.dat 10.0 0.3 0.1 k10_03b.dat 10.0 0.3 0.25 k10_03c.dat 10.0 0.3 0.5 k10_03d.dat 10.0 0.3 0.75 k10_03e.dat 10.0 0.3 1.0 k10_08a.dat 10.0 0.8 0.1 k10_08b.dat 10.0 0.8 0.25 k10_08c.dat 10.0 0.8 0.5 k10_08d.dat 10.0 0.8 0.75 k10_08e.dat 10.0 0.8 1.0 The files are ASCII data with two columns: Column 1: Log of frequency in Hz. Column 2: Log of rest frame monochromatic luminosity (nu Lnu) in erg/s