Felinic principle and measurement of the Hubble parameter
  Intelligent life can only appear in Universes, whose physical laws support
sufficient complexity to make evolution of intelligent beings possible. Even
inside those Universes, intelligent life does not appear randomly, but in parts
with realized complexity, e.g. around stars in our Universe. As a consequence,
the observational point of an intelligent observer cannot be assumed to be
random and one must correct for this selection effect. In this paper we
calculate how direct measurements of the Hubble parameter are affected when
subject to the condition that they are observed from a Milky Way-like galaxy.
