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   PR # 11106
    Mkn463E is a narrow line 'radio' galaxy.The X-ray luminosity expected
    from optical lines requires an extremely heavy absorption because it
    is not detected. The Einstein observation detected X-ray emission ,
    which is probably due to scattering emission as seen in NGC1068. The
    scientific goals are to get the first X-ray spectrum of Mkn463E and
    to examine whether Mkn463E is a first sample of NGC1068-type
    (=perfectly absorbed)quasars. 1E0449-184 is originally detected X-ray
    and then optically identified as the first narrow line quasar. In low
    luminous AGNs,'narrow line' almost always means 'absorption'. Does a
    high luminous AGN,1E0449-184, obey such a way too ? The goal is to
    investigate it.

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