  We present a detailed characterization of the X-ray spectral properties of
761 type 1 AGN, selected from a cross-correlation of the SDSS DR5 quasar
catalogue and the incremental version of the second XMM-Newton serendipitous
X-ray source catalogue 2XMMi-DR2. The X-ray spectrum of each source is fit with
models based on a simple power law to which additional cold absorption and/or
soft excess features are added if an F-test at 99% significance requires them.
The distribution of best-fitting photon indices, Gamma, is fit with a Gaussian
with mean <gamma> = 1.99 +/- 0.01 and dispersion sigma = 0.30 +/- 0.01, however
this does not provide a good representation of the distribution due to sources
with very flat or steep gamma values. A highly significant trend for decreasing
gamma values with increasing 2-10 keV luminosity, L_X, is seen but only a weak
trend with redshift is found. Intrinsic cold absorption is detected in ~4% of
the sample and soft excess emission is detected in ~8%. These values are lower
limits due to the detectability being limited by the quality of the spectra and
we suggest the intrinsic values may be as high as ~25% and ~80% respectively.
The levels of rest-frame absorption are higher than expected for type 1 objects
(N_H = 10^21-10^23 cm^-2) and the fraction of absorbed sources and the N_H
values are not seen to vary with L_X or z. The average blackbody temperature
used to model the soft excesses is <kT> = 0.17 +/- 0.09 keV. This temperature
is found to correlate with L_X but not the blackbody luminosity or the black
hole mass which do correlate with each other. A strong correlation is found
between the luminosities in the blackbody and power law components suggesting
that a similar fraction is re-processed from the blackbody to the power law
component for the entire luminosity range of objects. . . [Abridged]
