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   PR # 11119
    We propose observations of the two brightest broad line radio galaxie
    s(BLRGs) 3C120 and 3C382. The BLRGs are the low redshift counterparts
    to the radio loud quasars.Radio loud objects seem to be fundamentally
    different from radio quiet objects in that most of their luminosity
    is emitted in relativistic particles, yet the optical and ultraviolet
    spectra of these two classes are very similar. The largest observed
    difference between the these classes is seen in the x-ray spectra
    where the  radio loud objects are systematically flatter than that of
    radio quiet objects.  These high signal to noise data will be able to
    precisely determine the form of thee continuum, the nature of the
    soft excess seen in these objects and probably resolve the shape of
   the Fe K line.3C120
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