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   53017
   Recent investigations suggest that many of the observed differences
   between radio-loud AGN can be attributed to orientation dependent
   source properties. X-ray observations have revealed that radio-loud
   quasars with flat and steep radio spectra are also different in terms
   of their X-ray spectral index and their luminosity which could in
   principle be explained be a two component model for the X-ray emission.
   With this ASCA observation we want to investigate this two component
   model in detail by comparing the broad band X-ray spectrum of steep and
   flat spectrum radio quasars.
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