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   PR # 43032
   Comparison of the RASS with the (PG) survey has allowed the
   identification of 3 new BL Lacs, previously classified as white
   dwarfs, bringing to 6 the number of known BL Lacs in the complete
   optically-selected PG sample. All six objects are bright in the soft
   X-ray band ($\sim 10^{-11} erg/cm^2/sec$) but 2-10 keV data are
   lacking. We propose to observe with ASCA the two for which only RASS
   data are available (PG 1437+398, PG 1246+586), and PG 1424+240 for
   which the ROSAT data showed significan
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