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   PR #     7
   This region of the LMC contains a bright enhancement of diffuse
   emission whichcan be characterized as a superbubble breaking out of
   the plane of the galaxy.It is near to LMC X-1, which will be visible
   in the GIS during the observation.The calibration goal is to
   demonstrate that it is possible to subtract outthe extended wings of a
   bright source and study the diffuse emission by usingthe GIS spectrum
   and time variability of LMC X-1 to remove its influence fromthe SIS
   image. Scientifically, we want to characterize the spatially
   varyingspectral distribution of the hot diffuse gas to understand its
   origin.
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