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    PR # 31163                                                                   
     The extended X-ray/UV monitoring program of NGC5548 by Ginga and IUE        
     clearly indicated that the blue bamp, which had been interpretated as       
      the intrinsic thermal emission from an accretion disk, arised from t       
     he reprocessed X-ray, and showed importance of the reprocessing proce       
     ss in X-ray to UV region. We propose here a X-ray/UV/optical simultan       
     eous monitoring program of the bright Sefert I galaxy, Fairall-9. ASC       
     A has large advantage on X-ray spectroscopic research, and can accura       
     telly determine the flux and line profile of iron K-fluorescence emis       
     sion.  The observation proposed would be expected to reveal much abou       
     t the origine of blue bamp and iron K-emission to investivate the cor       
     relation of UV/X-ray continuum and iron K-emission reprocessed.             
                                                                                 
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