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   72141
   The as yet unexplained difference between radio-loud and radio-quiet
   active galaxies (AGNs) is a fundamental issue in our understanding of
   these objects. Eventhough a number of tantalizing correlations are
   known to exist between the radio and optical properties of AGNs, the
   situation in the X-ray band is unclear. Observations suggest systematic
   differences between the X-ray spectra of radio-quiet and radio-loud
   quasars, but it is unknown if these extend to the less luminous Seyfert
   and broad-line radio galaxies (BLRGs). We therefore propose to observe
   a few carefully-chosen BLRGs with the aim of measuring their continuum
   shape and Fe line properties. With these observations we will double
   the number of BLRGs observed by ASCA and compare their X-ray properties
   with those of Seyferts.
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