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   PR # 42122
   ESO198-G24 is a bright Seyfert galaxy which exhibits a complex and
   highly variable X-ray spectrum, yet this source has never been
   observed by ASCA. Some of the most significant recent advances in the
   AGN field have arisen from analysis of long observations of the
   brightest targets, thus we propose a 60 ksec observation of the
   ESO198-G24 field in order to study the source spectrum over a range
   of X-ray flux levels. This pointing will allow us to obtain a GIS
   spectrum of the AM Her system WWHOR, 25 arcmin away. This will allow
   the first significant constraint on the form of the hard X-ray
   component of the WWHOR spectrum.
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