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   51075
   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 is very strong
   and 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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