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   PR #    47
   There are two sources close together on the sky which are also
   bothX-ray pulsators. The pulsation periods are very similar (292
   and297s). One aim of this observation is to try and separate these
   twoclose (in position and period) sources. One of the sources
   (4U1145-61)flares to a very bright level with a 190 day period. If
   this source isin a flaring state it will be too bright for Asuka. If
   this is the case4U1145-61 will need to be offset out of the field of
   view.
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