Last updated: Sept 22, 2021

Contained in this directory are selected tabulated data for the work "Semi-analytic forecasts for JWST – V. AGN luminosity functions and helium reionization at z = 2 - 7" (accept for publication in MNRAS on Sept 21st, 2021).




The following directories contain the AGN one-point distribution functions presented in this work:

"AGN_LF_Bol" - AGN bolometric luminosity functions for our fiducial model (sigma_BH = 0.50), appeared as purple line in figure 8.

"AGN_LF_Bol_sig0.30" - AGN bolometric luminosity functions for the case where sigma_BH = 0.30, appeared as blue line in figure 8.

"AGN_LF_UV_intrinsic" - The intrinsic AGN UV luminosity functions (without obscuration or attenuation), appeared as dotted line in Figure 7.

"AGN_LF_UV_obscured" - The UV LFs for unobscured (Compton-Thin) AGN only, appeared as dashed line in Figure 7.

"AGN_LF_UV_dust" - The unobscured AGN UV LFs accounting for dust attenuation effects, appeared as solid line in Figure 7. Note that we provide the distribution of 500 independent realizations of dust attenuation. See text for more detail.

"AGN_LF_Xray_hard" - Hard x-ray AGN luminosity function for our fiducial model, appeared as purple dashed line in Figure 6.

"AGN_LF_Xray_soft" - Soft x-ray AGN luminosity function, not featured in publication	




The following directories contain scaling relations for hard ionizing photon production rate for AGN:

"mhalo_nHe" - ionizing photon production rate as a function of halo mass, as shown in Figure 17

"eps_nHe" - ionizing photon production rate as a function of specific emissivity at 1 ryd (912A), not featured in publication

"Mbol_nHe" - ionizing photon production rate as a function of bolometric luminosity, not featured in publication

"mdot_nHe" - ionizing photon production rate as a function of black hole accretion rate, not featured in publication





For more details see Yung et al. 2021 and reference