Observational Constraints on Very Faint, High-z, Quasars

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Scientific paper

I will discuss the constraints that can be derived on the abundance of
high redshift (z>6) miniquasars and regular quasars from the
unresolved soft X-Ray background. Furthermore, I will show how data
generated by existing Lyman alpha surveys can be used to constrain the
very faint (M_B~-16) end of the high-z quasar luminosity function.

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