  We report our analysis of X-ray spectra of the Seyfert galaxy IRAS 18325-5926
(=Fairall 49) obtained from various X-ray observatories prior to XMM-Newton,
including new results from two RXTE and one BeppoSAX observations. A relatively
steep continuum slope (photon-index of ~2.2) in the 2-15 keV band is confirmed.
The continuum spectrum observed with the BeppoSAX PDS shows a possible
roll-over at energies above 30 keV, indicating a Comptonizing corona cooler
than in other Seyfert nuclei. The X-ray spectrum above 2 keV is best explained
with a model including reflection from a highly ionized disk with significant
relativistic blurring. The iron K-alpha emission feature is then mainly due to
FeXXV. The recent seven observations shows that the iron K emission flux
appears to follow the continuum between the observations separated by a few
months to years, although some exceptions suggest that the line strength may be
determined in a more complex way.
