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   PR #    99
   IRAS 18325-5926 has been classified as Seyfert 2 galaxies in the
   opticalband. In the Unified Seyfert model, the nucleus of the Seyfert
   2 galaxywould be obscured by the surrounding thick matter so called an
   accretion torus. However we can not find any evidence of the
   obscuration in Ginga obervation. The purpose of this observation is a
   test of the Unified Seyfert Model.
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