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   PR # 41171
   We observe one of the two peaks of the QSO cluster (z=1.0-1.2)
   discovered by Crampton et al. 1989. The other peak was observed with
   ASCA in 1995 as AO-3 target with 100 ksec exposure. Our preliminal
   analysis of the data suggests that observing the QSO cluster region
   is indeed very fruitful. 1. We may detect more QSOs than a blank sky
   survey in a field of view. We can not only compair Lx and Lopt but
   also obtain distribution of the X-ray hardness-ratio for QSOs at the
   same redshift. 2. We have much more chance to discover "Type-2 QSO"
   than in general field, since they may be in the same distribution as
   the ordinary optical QSO.
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