  Evidence of excess GeV emission nearly coinciding with the Galactic Centre
has been interpreted as a possible signature of annihilating dark matter. In
this paper, we argue that it seems too early to discard pulsars as a viable
explanation for the observed excess. On the heels of the recently released
Second Fermi LAT Pulsar Catalogue (2FPC), it is still possible that a
population of hard (Gamma < 1) millisecond pulsars (MSPs) either endemic to the
innermost region or part of a larger nascent collection of hard MSPs that
appears to be emerging in the 2FPC could explain the GeV excess near the
Galactic Centre.
