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   PR #    21
   The Scientfic goals are to obtain the best broadband X-ray spectrum to
   date of the Seyfert II Galaxy MKN 3 and to better characterize the Fe
   K and L emission features detected by BBXRT. Wheres the GINGA spectrum
   is heavily cutoff, the continuum rises again at lower energies,
   suggesting a scattered or leakage component below 3 keV. A broadband
   spectrum from ASUKA is necessaryto constrain the continuum shape and
   line features. Main calibration goal is the spectroscopy of faint
   sources.
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