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   52141
   3C321 is one of very few examples of a NLRG in which an obscured quasar
   has been demonstrated to exist. Its extended continuum polarization
   properties are similar to those of Cygnus A, but also shows polarized
   emission from the BLR in the visible. It is of importance to observe it
   at hard X-ray energies, since we only have indirect estimates for the
   luminosity of its obscured nucleus. Unlike Seyfert AGN, currently the
   statistics on hard X-ray properties of powerful NLRGs are extremely
   sparse. The proposed observations will show whether 3C321's hard X-ray
   properties are similar to those of Seyfert 2s observed by Asca, or
   whether it is like NGC1068, with an extremely high absorbing column.
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