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    PR # 31127                                                                   
       We propose to observe two LLAGN candidates NGC5033 and NGC4450.  Th       
     ey have optical spectra intermidiate between LINERs and  Seyferts whi       
     ch are suitable to investigate the LLAGN phenomena  and their evoluti       
     onary relations to usual Seyferts and QSOs. We  attempt to probe a mo       
     nster using broad band Spectra and time  variability which are availa       
     ble by ASCA high sensitivity for the  first time. We hope to clarify        
     whether LLAGN hosts a hungry  monster or a small monster. Our furhter       
      understanding of LLAGN   natures also leads to give a hint of origin       
      of Cosmic X-ray  Background.                                               
                                                                                 
                                                                                 
                                                                                 
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