  In an analysis of XMM-Newton archival observations of the bright Local Group
spiral galaxy M 31 we study the population of X-ray sources (X-ray binaries,
supernova remnants) down to a 0.2-4.5 keV luminosity of 4.4E34 erg/s. EPIC
hardness ratios and optical and radio information are used to distinguish
between different source classes. The survey detects in an area of 1.24 square
degree 856 sources. We correlate our sources with earlier M 31 X-ray catalogues
and use information from optical, infra-red and radio wavelengths. As M 31
sources we detect 21 supernova remnants (SNR) and 23 SNR candidates, 18
supersoft source (SSS) candidates, 7 X-ray binaries (XRBs) and 9 XRB
candidates, as well as 27 globular cluster sources (GlC) and 10 GlC candidates,
which most likely are low mass XRBs within the GlC. Comparison to earlier X-ray
surveys reveal transients not detected with XMM-Newton, which add to the number
of M 31 XRBs. There are 567 sources classified as hard, which may either be
XRBs or Crab-like SNRs in M 31 or background AGN. The number of 44 SNRs and
candidates more than doubles the X-ray detected SNRs. 22 sources are new SNR
candidates in M 31 based on X-ray selection criteria. Another SNR candidate may
be the first plerion detected outside the Galaxy and the Magellanic Clouds. On
the other hand, six sources are foreground stars and 90 foreground star
candidates, one is a BL Lac type active galactic nucleus (AGN) and 36 are AGN
candidates, one source coincides with the Local Group galaxy M 32, one with a
background galaxy cluster (GCl) and another is a GCl candidate, all sources not
connected to M 31.
