Future work

• Alternatives to LDDE (Ueda+14) LF
• Parameterisation of obscuration & its evolution
• Tighter constraints by more knowledge (broken powerlaws)
• Sołtan argument integration
• Does the luminosity output match the local black hole mass density?
• XRB predictions
• Including additional reflection
• Integrate the local BHMF backwards
• BHMF at higher redshifts
• Eddington rate distribution at higher redshifts