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   81652
   Large Magelanic Cloud has extremely ideal characters for the systematic
   study of X-ray sources.  The aims and expected fruit of this survey are
   (1) Comprehensive study of X-ray source populations, which reflect the
   star-formation history in the Magellanic Clouds, (2) Discovery of new
   X-ray pulsars, (3) Discovery of non-thermal X-ray emission from SNRs,
   which leads to a quantitative estimation of cosmic ray acceleration in
   SNRs,and (4) To obtain the complete X-ray images including both
   discrete sources and diffuse X-rays. In the Post-AO8 phase, we will
   observe six regions where bright ROSAT sources remain to be observed.
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