  We present first results from a 325 ks observation of the Seyfert 1 galaxy
MCG-6-30-15 with XMM-Newton and BeppoSAX. The strong, broad, skewed iron line
is clearly detected and is well characterised by a steep emissivity profile
within 6r_g (i.e. 6GM/c^2) and a flatter profile beyond. The inner radius of
the emission appears to lie at about 2r_g, consistent with results reported
from both an earlier XMM-Newton observation of MCG-6-30-15 by Wilms et al. and
part of an ASCA observation by Iwasawa et al. when the source was in a lower
flux state. The radius and steep emissivity profile do depend however on an
assumed incident power-law continuum and a lack of complex absorption above 2.5
keV. The blue wing of the line profile is indented, either by absorption at
about 6.7 keV or by a hydrogenic iron emission line. The broad iron line flux
does not follow the continuum variations in a simple manner.
