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Using the fundamental plane to unveil the history of accretion I: The local population
At redshift zero, we do have the hard XLF (Ueda et al. 2003), the AGN RLF (Sadler et al. 2002; Willott et al. 2001) and the BHMF (Aller and Richstone 2003, Yu and Tremaine 2002).
It is possible then to find an appoximated conditional LF such that the following integral constraints are fulfilled: