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   PR # 11154
     We propose to use ASCA to observe the brightest radio quiet QSO at
    redshift greater than 1 to search for the reflection signatures, an
    iron line and reflection hump,present in lower luminosity,nearby AGN.
    The high sensitivity of ASCA means that reasonable spectra can be
    obtained in 40ks, and at high zthe reflection hump is redshifted into
    the ASCA bandpass. These observations offer an opportunity to probe
    the accretion flow in high redshift QSO and test evolutionary
    theories.




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