Untangling the White Dwarf Luminosity Functions
  The inversion of the white dwarf luminosity function provides an independent
way to prove the past star formation history of the Milky Way independent of
any cosmological models. In Rowell & Hambly (2011), the effective volume method
uses the average properties of all the objects in a given bin, so a significant
amount of information is lost in the early stage of the analysis, in this work,
I explore the possibility of assigning objects individually in a probabilistic
way using the generalised Schmidt density estimator (1/Vmax).
