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   63025
   Our new, soft-X-ray-selected, dusty warm-absorber candidate
   IRAS12397+3333 shows a unique set of properties, linking three of the
   most interesting phenomena in AGN research: the FeII problem, the
   nature and location of warm absorbers, and the role of Unified Schemes.
   It is a Narrow Line Sey 1, unexpectedly dusty for its high luminosity
   (1E11 Lsuns). It shows high optical reddening and scattering
   polarization up to 7%, implying aspect-dependent views. Lack of cold
   absorption in its steep, rapidly-variable soft-X-ray spectrum hints at
   warm dusty absorbers - consistent with its complex ROSAT spectrum. With
   our spectropolarimetry, our proposed ASCA measurement of the probable
   warm absorbers, and the 0.5 - 9 keV continuum, will allow a powerful
   probe of parsec-scale dusty ionized gas.
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