Spectral Energy Distribution 
[1um-0.1keV only contains AGN SED; others are the star-formation and AGN combined]: 

log(NHI)               :     
0.0                 
21.5                
22.5                
23.5                
24.5                
25.5                
 (HI column to extinguish the AGN radiation) 


log(LTIR)a             :     8-1000 um luminosity in log(Lsun)
 

log(Lbh/Ltot)TIR        :     The logarithm of the fractional SMBH energy 
                                     in the 8-1000 um (minimum: -6, maximum: 0)
 


log(Star Formation Colorb) :    
-3.0                 
-2.5                
-2.0                
-1.5                
-1.0                
-0.5                
 0.0                
 0.5                
 1.0                
 1.5                
 2.0                
 2.5                
 3.0                 




   

aFor AGN SED with no star formation (i.e., log(Lbh/Ltot)=0) and no extinction, 
            log(LTIR) = -1.288+1.181xlog(Lbol) - 0.012xlog(Lbol)2
            log(LTIR) = -0.314+1.110xlog(L2-10keV) 

bAt a given star-formation IR luminosity, the star-formation color distribution is 
            a Gaussian function (Chapman et al. 2003). The input value gives the offset from 
            the mean in the unit of the Gaussian width, e.g. an input value of 2.0 gives 2σ
            away from the mean color.