On the redshift of the blazar PKS0447-439
  PKS0447-439 is one of the BL Lacertae objects that have been detected at very
high energy. There has been a recent report of a lower limit of z>1.246 for the
redshift of this blazar, challenging the current paradigm in which very
high-energy gamma-rays cannot freely propagate in the z>1 universe. In this
research note, we present a new MagE/Magellan spectrum of PKS0447-439 with
exquisite signal-to-noise (S/N>150 at 6500A). Our analysis confirms the
presence of the previously-reported absorption line at 6280A, which we
identify, however, with a known telluric absorption, invalidating the claim
that this blazar lies at z>1. Since no other extragalactic spectral features
are detected, we cannot establish a redshift based on our spectrum.
