AGN Populations from Optical Identification of ASCA Surveys
  To understand luminous AGNs in the z<1 universe, the ASCA AGN samples are the best at present. Combining the identified sample of AGNs from ASCA Large Sky Survey and Medium Sensitivity Survey, the sample of hard X-ray selected AGNs have been expanded up to 108 AGNs above the flux limit of 10^{-13} erg s^{-1} cm^{-2} in the 2-10 keV hard X-ray band. We discuss the fraction of absorbed AGNs in the hard X-ray selected AGN sample, and nature of absorbed luminous AGNs. 
Masayuki Akiyama (Subaru Telescope, NAOJ), Yoshihiro Ueda (ISAS),   Kouji Ohta (Dept. of Astronomy, Kyoto University)