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   We propose to observe the 6 remaining sources out of the 20 hard X-ray
   selected broad emission-line (BEL) AGN (Seyfert 1s and quasars) in the
   Piccinotti sample, not yet observed with ASCA. This complete, well-
   defined sample, unbiased with respect to radio/ infrared/ optical/ UV/
   soft X-ray properties will provide a solid basis for systematic
   investigation of the X-ray spectral properties and therefore inferred
   physical properties. In particular we will investigate the properties
   of the photoionized absorbers and complex Fe-K lines commonly found in
   other BEL AGN. The ASCA Piccinotti sample will be unprecedented in
   sensitivity and spectral resolution and will provide the data for key
   statistical tests and theoretical models. Continued CCD damage makes
   completion of this sample very urgent.
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