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).
Local blackbody emission is assumed.




The files are:

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

k6_01_01.dat		6.0		0.1		  0.1
k6_01_025.dat		6.0		0.1		  0.25
k6_01_05.dat		6.0		0.1		  0.5	
k6_01_075.dat 		6.0		0.1		  0.75
k6_01_1.dat		6.0		0.1		  1.0

k6_03_01.dat		6.0		0.3	   	  0.1
k6_03_025.dat		6.0		0.3		  0.25
k6_03_05.dat		6.0		0.3		  0.5
k6_03_075.dat		6.0		0.3  		  0.75
k6_03_1.dat		6.0		0.3		  1.0

k6_08_01.dat		6.0		0.8 		  0.1
k6_08_025.dat		6.0		0.8		  0.25
k6_08_05.dat		6.0		0.8		  0.5
k6_08_075.dat		6.0		0.8		  0.75	
k6_08_1.dat		6.0		0.8		  1.0

k6_1_01.dat		6.0		1.0		  0.1
k6_1_025.dat		6.0		1.0		  0.25
k6_1_05.dat		6.0		1.0		  0.5
k6_1_075.dat		6.0		1.0		  0.75	
k6_1_1.dat		6.0		1.0		  1.0

k7_01_01.dat		7.0		0.1		  0.1
k7_01_025.dat		7.0		0.1		  0.25
k7_01_05.dat		7.0		0.1		  0.5	
k7_01_075.dat 		7.0		0.1		  0.75
k7_01_1.dat		7.0		0.1		  1.0

k7_03_01.dat		7.0		0.3	   	  0.1
k7_03_025.dat		7.0		0.3		  0.25
k7_03_05.dat		7.0		0.3		  0.5
k7_03_075.dat		7.0		0.3  		  0.75
k7_03_1.dat		7.0		0.3		  1.0

k7_08_01.dat		7.0		0.8 		  0.1
k7_08_025.dat		7.0		0.8		  0.25
k7_08_05.dat		7.0		0.8		  0.5
k7_08_075.dat		7.0		0.8		  0.75	
k7_08_1.dat		7.0		0.8		  1.0

k7_1_01.dat		7.0		1.0		  0.1
k7_1_025.dat		7.0		1.0		  0.25
k7_1_05.dat		7.0		1.0		  0.5
k7_1_075.dat		7.0		1.0		  0.75	
k7_1_1.dat		7.0		1.0		  1.0


k8_01_01.dat		8.0		0.1		  0.1
k8_01_025.dat 		8.0		0.1		  0.25
k8_01_05.dat		8.0		0.1		  0.5
k8_01_075.dat		8.0		0.1 		  0.75
k8_01_1.dat		8.0		0.1		  1.0

k8_03_01.dat		8.0		0.3 		  0.1
k8_03_025.dat		8.0		0.3		  0.25		
k8_03_05.dat		8.0		0.3		  0.5
k8_03_075.dat		8.0		0.3		  0.75
k8_03_1.dat		8.0		0.3		  1.0

k8_08_01.dat		8.0		0.8		  0.1	
k8_08_025.dat		8.0		0.8		  0.25
k8_08_05.dat		8.0		0.8		  0.5
k8_08_075.dat		8.0		0.8		  0.75
k8_08_1.dat		8.0		0.8		  1.0

k8_1_01.dat		8.0		1.0		  0.1	
k8_1_025.dat		8.0		1.0		  0.25
k8_1_05.dat		8.0		1.0		  0.5
k8_1_075.dat		8.0		1.0		  0.75
k8_1_1.dat		8.0		1.0		  1.0

k9_001_01.dat		9.0		0.01		  0.1
k9_001_025.dat		9.0		0.01		  0.25
k9_001_05.dat		9.0		0.01		  0.5
k9_001_075.dat		9.0		0.01		  0.75
k9_001_1.dat		9.0		0.01		  1.0

k9_01_01.dat		9.0		0.1		  0.1
k9_01_025.dat		9.0		0.1		  0.25
k9_01_05.dat		9.0		0.1		  0.5
k9_01_075.dat		9.0		0.1		  0.75
k9_01_1.dat		9.0		0.1		  1.0

k9_03_01.dat		9.0		0.3		  0.1
k9_03_025.dat		9.0		0.3		  0.25
k9_03_05.dat		9.0		0.3		  0.5
k9_03_075.dat		9.0		0.3		  0.75
k9_03_1.dat		9.0		0.3		  1.0

k9_08_01.dat		9.0		0.8		  0.1
k9_08_025.dat		9.0		0.8		  0.25
k9_08_05.dat		9.0		0.8		  0.5
k9_08_075.dat		9.0		0.8		  0.75
k9_08_1.dat		9.0		0.8		  1.0

k9_1_01.dat		9.0		1.0		  0.1
k9_1_025.dat		9.0		1.0		  0.25
k9_1_05.dat		9.0		1.0		  0.5
k9_1_075.dat		9.0		1.0		  0.75
k9_1_1.dat		9.0		1.0		  1.0

k10_001_01.dat		10.0		0.01		  0.1
k10_001_025.dat		10.0		0.01		  0.25
k10_001_05.dat		10.0		0.01		  0.5
k10_001_075.dat		10.0		0.01		  0.75
k10_001_1.dat		10.0		0.01		  1.0

k10_01_01.dat		10.0		0.1		  0.1
k10_01_025.dat		10.0		0.1		  0.25
k10_01_05.dat		10.0		0.1		  0.5
k10_01_075.dat		10.0		0.1		  0.75
k10_01_1.dat		10.0		0.1		  1.0

k10_03_01.dat		10.0		0.3		  0.1
k10_03_025.dat		10.0		0.3		  0.25
k10_03_05.dat		10.0		0.3		  0.5
k10_03_075.dat		10.0		0.3		  0.75
k10_03_1.dat		10.0		0.3		  1.0

k10_08_01.dat		10.0		0.8		  0.1
k10_08_025.dat		10.0		0.8		  0.25
k10_08_05.dat		10.0		0.8		  0.5
k10_08_075.dat		10.0		0.8		  0.75
k10_08_1.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








