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   51208
   We propose observations of Pisces-Perseus supercluster at the middle
   regions of Perseus cluster (z=0.0183) and AWM7 (z=0.0179), with 3
   pointings of each 30 ks. Our prompt objective is to detect the X-ray
   emission from the supercluster of galaxies for the first time. Both
   Perseus and AWM7 are bright in X-ray and have elongated shapes along
   the supercluster axis, so that the Xray detection is quite probable. If
   the temperature and/or abundance are measured, it will give an
   important implications about the formation of the large scale structure
   of the Universe, etc.
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