Figure 11
Observed 0.5–2 keV flux from a BH with the Hopkins et al. (2007) SED shining at its Eddington limit as a function of source redshift. BH masses as labelled.
Observed 0.5–2 keV flux from a BH with the Hopkins et al. (2007) SED shining at its Eddington limit as a function of source redshift. BH masses as labelled.
