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   73021
   Contrary to radio-quiet AGN, the evidence for an accretion disk in
   radio-loud AGN is, at most, sparse. In particular, Fe-K line emission
   around 6.4 keV is either absent or only marginally detected. On the
   other hand, double-peaked H alpha emission has been discovered in a few
   radio-loud AGN. The most promising explanation for the double-peaked
   structure is that the emission line originates in the putative
   accretion disk. Here we propose to observe two low-luminosity double-
   peaked radio galaxies to search for the X-ray signatures of an
   accretion disk. Our observation will not only be relevant for double-
   peaked AGN, but will further enhance our knowledge on the innermost
   region of radio-loud AGN in general and the enigmatic radio-loud/radio-
   quiet dichotomy.
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