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   Soft X-ray selection picks out unabsorbed objects which have strong
   "soft excesses". This energetically important component, likely the
   high energy tail of the accretion disk spectrum, plays an important
   role in production of optical emission lines and hard X-ray spectra.
   Proposed ASCA observations of the 8 remaining objects in a complete
   sample of 19 soft X-ray selected AGN will yield hard X-ray spectra and
   variability information. Statistical analysis of these results with an
   existing database of multiwaveband and optical properties will be
   performed. Coordinated EUVE observations will yield simultaneous soft
   X-ray light curves. These results will allow us to significantly
   advance our understanding of the relationships between the soft excess,
   multiwaveband,
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