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.
@article{arxiv.1207.3592,
title = {On the redshift of the blazar PKS0447-439},
author = {Michele Fumagalli and Amy Furniss and John M. O'Meara and J. Xavier Prochaska and David A. Williams and Emanuele P. Farina},
journal= {arXiv preprint arXiv:1207.3592},
year = {2012}
}