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   PR # 11127
      With the Ginga observations, we found that the central engines of
    NGC4507 (Seyfert 2 galaxy) and IC5063 (Narrow line radio galaxy)  are
    found to be surrounded by geometically and optically thick torus, and
    X-rays are heavily absorbed.  With SIS, which has high energy
    resolusion and broad energy band, we intend to observe both emissions
    of absorbed (hard X-ray) and scattered components (soft X-ray).  We
    will aslo clarify whether soft-x-rays are scattered one or thermal
    emission of the  host galaxy. Fe K-line emission would be powerful
    diagnostics for the physical condition of accretion torus or disk.



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