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   We propose the extreme Fe II quasar PHL 1092 to study its high energy
   continuum and strong variability. PHL 1092 is a high-luminosity narrow-
   line Seyfert 1 class object, and its ROSAT spectrum is extremely soft.
   ASCA will let us study its high energy spectrum for the first time to
   determine if it is different from that of more typical quasars. PHL
   1092 shows large amplitude and remarkably rapid variability in its
   ROSAT observation, and it may also show giant amplitude X-ray
   variability. Our observation will study the variability better than
   ever before. It is very important to study the spectra of unusual
   quasars like PHL 1092 to explore the extremes of quasar behavior and
   expand the spectral window function.
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