Accretion Disk Models in the Schwarzschild 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).
Assumed modified blackbody emission (electron scattering and
Comptonization in the disk's atmosphere).




The files are:

Filename       Model Parameters
-----------------------------------------------------------------------------
		Log Black Hole Mass     Accretion Rate    Inclination Angle
		(in solar mass)  	(in Eddington)       (cos theta)
						

s6_01a.dat  		6.0		0.1		  0.1
s6_01b.dat   		6.0		0.1		  0.25
s6_01c.dat  		6.0		0.1		  0.5	
s6_01d.dat    		6.0		0.1		  0.75
s6_01e.dat 		6.0		0.1		  1.0

s6_03a.dat  		6.0		0.3	   	  0.1
s6_03b.dat   		6.0		0.3		  0.25
s6_03c.dat  		6.0		0.3		  0.5
s6_03d.dat   		6.0		0.3  		  0.75
s6_03e.dat 		6.0		0.3		  1.0

s6_08a.dat  		6.0		0.8 		  0.1
s6_08b.dat   		6.0		0.8		  0.25
s6_08c.dat  		6.0		0.8		  0.5
s6_08d.dat   		6.0		0.8		  0.75	
s6_08e.dat 		6.0		0.8		  1.0


s7_01a.dat  		7.0		0.1		  0.1
s7_01b.dat   		7.0		0.1		  0.25
s7_01c.dat  		7.0		0.1		  0.5	
s7_01d.dat    		7.0		0.1		  0.75
s7_01e.dat 		7.0		0.1		  1.0

s7_03a.dat  		7.0		0.3	   	  0.1
s7_03b.dat   		7.0		0.3		  0.25
s7_03c.dat  		7.0		0.3		  0.5
s7_03d.dat   		7.0		0.3  		  0.75
s7_03e.dat 		7.0		0.3		  1.0

s7_08a.dat  		7.0		0.8 		  0.1
s7_08b.dat   		7.0		0.8		  0.25
s7_08c.dat  		7.0		0.8		  0.5
s7_08d.dat   		7.0		0.8		  0.75	
s7_08e.dat 		7.0		0.8		  1.0


s8_01a.dat  		8.0		0.1		  0.1
s8_01b.dat    		8.0		0.1		  0.25
s8_01c.dat  		8.0		0.1		  0.5
s8_01d.dat   		8.0		0.1 		  0.75
s8_01e.dat 		8.0		0.1		  1.0

s8_03a.dat  		8.0		0.3 		  0.1
s8_03b.dat   		8.0		0.3		  0.25		
s8_03c.dat  		8.0		0.3		  0.5
s8_03d.dat   		8.0		0.3		  0.75
s8_03e.dat 		8.0		0.3		  1.0

s8_08a.dat  		8.0		0.8		  0.1	
s8_08b.dat   		8.0		0.8		  0.25
s8_08c.dat  		8.0		0.8		  0.5
s8_08d.dat   		8.0		0.8		  0.75
s8_08e.dat 		8.0		0.8		  1.0


s9_01a.dat  		9.0		0.1		  0.1
s9_01b.dat   		9.0		0.1		  0.25
s9_01c.dat  		9.0		0.1		  0.5
s9_01d.dat   		9.0		0.1		  0.75
s9_01e.dat 		9.0		0.1		  1.0

s9_03a.dat  		9.0		0.3		  0.1
s9_03b.dat   		9.0		0.3		  0.25
s9_03c.dat  		9.0		0.3		  0.5
s9_03d.dat   		9.0		0.3		  0.75
s9_03e.dat 		9.0		0.3		  1.0

s9_08a.dat  		9.0		0.8		  0.1
s9_08b.dat   		9.0		0.8		  0.25
s9_08c.dat  		9.0		0.8		  0.5
s9_08d.dat   		9.0		0.8		  0.75
s9_08e.dat 		9.0		0.8		  1.0


s10_001a.dat  		10.0		0.01		  0.1
s10_001b.dat   		10.0		0.01		  0.25
s10_001c.dat  		10.0		0.01		  0.5
s10_001d.dat   		10.0		0.01		  0.75
s10_001e.dat 		10.0		0.01		  1.0

s10_01a.dat  		10.0		0.1		  0.1
s10_01b.dat   		10.0		0.1		  0.25
s10_01c.dat  		10.0		0.1		  0.5
s10_01d.dat   		10.0		0.1		  0.75
s10_01e.dat 		10.0		0.1		  1.0

s10_03a.dat  		10.0		0.3		  0.1
s10_03b.dat   		10.0		0.3		  0.25
s10_03c.dat  		10.0		0.3		  0.5
s10_03d.dat   		10.0		0.3		  0.75
s10_03e.dat 		10.0		0.3		  1.0

s10_08a.dat  		10.0		0.8		  0.1
s10_08b.dat   		10.0		0.8		  0.25
s10_08c.dat  		10.0		0.8		  0.5
s10_08d.dat   		10.0		0.8		  0.75
s10_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