  The participants in this meeting are almost all carrying out the hard work of
making many different types of AGN surveys. Since it's so much easier to
criticize other people's work than to do actual work myself, I'll just present
some demurs regarding recent papers drawing conclusions from various AGN survey
data. In particular I'll mention some questionable interpretations of surveys
of Seyfert 2 near-UV polarization; interpreting the results of searches for
polarized broad H-alpha lines in Seyfert 2s; testing the beam model for radio
galaxies and quasars; testing the unification of Seyfert spectral types with a
torus; and finally testing the energy sources for Ulirgs, especially those with
Liner optical spectra. Only the polarized broad H-alpha results are examined in
detail here.
