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   PR # 41139
   We propose observations of the ultraluminous IRAS galaxies IRAS
   00235+1024 and IRAS 23060+0505 to search for hidden AGN and advance
   Seyfert/quasar/ultraluminous IRAS galaxy unification. Both objects
   have luminosities characteristic of quasars and show evidence for
   obscuring material. They may have fluorescent line emission which
   would indicate the reprocessing of X-rays from a central AGN.
   IRAS00235+1024 was recently discovered to be the third most
   luminousIRAS galaxy known during a Cambridge APM machine systematic
   survey. IRAS 23060+0505 is both nearby and powerful so we should be
   able to probe it in detail.
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