  In a recent paper (arXiv:1612.00266), we reported the results of the first
search for echoes from Planck-scale modifications of general relativity near
black hole event horizons using the public data release by the Advanced LIGO
gravitational wave observatory. While we found tentative evidence (at $\simeq 3
\sigma$ level) for the presence of these echoes, our statistical methodology
was challenged by Ashton, et al. (arXiv:1612.05625), just in time for the
holidays! In this short note, we briefly address these criticisms, arguing that
they either do not affect our conclusion or change its significance by
$\lesssim 0.3\sigma$. The real test will be whether our finding can be
reproduced by independent groups using independent methodologies (and
ultimately more data).
