Home Spectral Energy Distributions Number Counts Redshift Distributions Luminosity Functions Comoving Number Density With z 6.2um PAH Equivalent Width Distribution Background Light Spectrum

The  model aims to constrain     supermassive black-hole accretion     dusty star formation by parametrizing    luminosity functions in the total IR band,    SMBH energy fraction as a function of the IR luminosity,    HI column density to obscure SMBH accretion. The best-fit parameters are derived by fitting 617 data points of     number counts in X-ray and IR bands     redshift distributions in X-ray and IR bands     local luminosity functions in X-ray and IR bands. Contact: yshipku [at] gmail [dot] com Reference: Shi et al. 2013 [arXiv]