*************************************************************************
   51176
   The broad Fe K line profile found in AGN spectra is the most important
   result to investigate accretions discs around massive blackholes. Among
   many AGN's with such line feature, the line width and equivalent width
   is largest for IRAS18325-5926. In the spectra observed in the PV phase,
   the high energy side of the line profile extends up to 7 keV, which
   suggests highly ionized ions or larger inclination angle. It is worth
   observing IRAS18325 as long as 200 ksec to conclude it with enough
   statistics. It has been also reported that the broad line feature
   changes during the total flux change. We propose to observe IRAS18325
   for 200 ksec to monitor the flux change as well as the change of line
   profile to examine the disc size, structure and its physical status.
 *************************************************************************