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   52138
   A 40 ks ASCA observation of the unabsorbed and presumably face-on
   Seyfert 1 galaxy MCG-2-58-22 is proposed. Our primary goals are to
   study the continuum shape and determine the Fe Kalpha line profile (and
   possibly variability if the source is in a high flux state) in
   conjunction with XTE at a level that is not possible with existing PV
   data. The current ASCA data allow no useable constraints to be placed
   on the iron line parameters. We will also monitor the long-term flux
   variability of the line-like soft excess that almost disappeared
   between the Einstein and ASCA observations spaced 14 years apart.
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