The Galactic neutron star population I - an extragalactic view of the
  Milky Way and the implications for fast radio bursts
  A key tool astronomers have to investigate the nature of extragalactic
transients is their position on their host galaxies. Galactocentric offsets,
enclosed fluxes and the fraction of light statistic are widely used at
different wavelengths to help infer the nature of transient progenitors.
Motivated by the proposed link between magnetars and fast radio bursts (FRBs),
we create a face-on image of the Milky Way using best estimates of its size,
structure and colour. We place Galactic magnetars, pulsars, low mass and high
mass X-ray binaries on this image, using the available distance information.
Galactocentric offsets, enclosed fluxes and fraction of light distributions for
these systems are compared to extragalactic transient samples. We find that
FRBs follow the distributions for Galactic neutron stars closest, with 24 (75
per cent) of the Anderson-Darling tests we perform having a p-value greater
than 0.05. This suggests that FRBs are located on their hosts in a manner
consistent with Galactic neutron stars on the Milky Way's light, although we
cannot determine which specific neutron star population is the best match. The
Galactic distributions are consistent with other extragalactic transients much
less often across the range of comparisons made, with type Ia SNe in second
place, at only 33 per cent of tests exceeding 0.05. Overall, our results
provide further support for FRB models invoking isolated young neutron stars,
or binaries containing a neutron star.
