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   PR #   111
   NGC5548 is a bright Seyfert Galaxy and has been observed extensively
   in various wave bands. In X-ray band, Iron K flourecent line (E.W. 130
   eV) ,edge structure, and soft-excess was observed. Higher energy
   resolution spectrum with ASCA will provide us a clue to several
   proposed models on the structure of the central X-ray emission region
   and its surroundigs.
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