*************************************************************************
   81603
   Large and Small Magelanic Clouds have 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. A new X-ray view of
   the Magellanic Clouds will be established through this survey.
 *************************************************************************