  Initial results on the iron K-shell line and reflection component in several
AGN observed as part of the Suzaku Guaranteed time program are reviewed. This
paper discusses a small sample of Compton-thin Seyferts observed to date with
Suzaku; namely MCG -5-23-16, MCG -6-30-15, NGC 4051, NGC 3516, NGC 2110, 3C 120
and NGC 2992. The broad iron K$\alpha$ emission line appears to be present in
all but one of these Seyfert galaxies, while the narrow core of the line from
distant matter is ubiquitous in all the observations. The iron line in MCG
-6-30-15 shows the most extreme relativistic blurring of all the objects, the
red-wing of the line requires the inner accretion disk to extend inwards to
within 2.2Rg of the black hole, in agreement with the XMM-Newton observations.
Strong excess emission in the Hard X-ray Detector (HXD) above 10 keV is
observed in many of these Seyfert galaxies, consistent with the presence of a
reflection component from reprocessing in Compton-thick matter (e.g. the
accretion disk). Only one Seyfert galaxy (NGC 2110) shows neither a broad iron
line nor a reflection component. The spectral variability of MCG -6-30-15, MCG
-5-23-16 and NGC 4051 is also discussed. In all 3 cases, the spectra appear
harder when the source is fainter, while there is little variability of the
iron line or reflection component with source flux. This agrees with a simple
two component spectral model, whereby the variable emission is the primary
power-law, while the iron line and reflection component remain relatively
constant.
