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   71063
   We discovered an X-ray emission from supernova remnant G352.7-0.1,
   during the galactic plane survey program performed in the AO-4 period
   for the first time. The diameter was about 6-8 arcmin. The X-ray
   spectrum shows that emission lines from Si, S, and Ar are very strong.
   The GIS spectrum and image imply that there is a point-like source at
   the center. However, since the exposure time during the survey program
   was short, we could not obtain statistically good data. Thus, we
   propose a follow-up observation of this supernova remnant.
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