******************************************************
   PR # 43027
   `Narrow-line' Seyfert 1 galaxies possess steep soft X-ray slopes
   compared to the mean for Seyfert 1 type galaxies as well as rapid and
   large amplitude X-ray variability. We propose the bright narrow-line
   and extreme Fe II Seyfert 1 galaxy PKS 0558-504. We will measure the
   shape and luminosity of the strong soft excess as well as the break
   energy where the hard tail takes over from the soft component. We
   will quantify the amounts of hard and soft flux to determine whether
   the soft excess might plausibly be produced by hard X-ray
   reprocessing. PKS 0558-504 is known to be variable and we will search
   for spectral variability. We will sensitively probe iron K line
   emission in PKS 0558-504 to examine the iron line dichotomy between
   Seyferts and quasars.
  ******************************************************