*************************************************************************
   62115
   We propose six 30ks ASCA observations of the bright Seyfert 1 galaxy
   NGC5548 over a period of 20-40 days. Along with coordinated RXTE
   observations, a 30ks integration will allow us to measure the warm
   absorption features, the broad iron fluorescence line, and the
   `reflected' continuum. We will search for variability of the iron line
   profile/strength and study the physical implications for any such
   variability on the nature of the inner disk. The instantaneous iron-
   line/reflection-continuum form will constrain the iron abundance and
   probe the absolute normalization of the reflection component. Our
   temporal study of the warm absorption features will allow the location
   of this material to be constrained, allowing us to relate the warm
   absorber to other known structures.
 *************************************************************************