  Using the Spitzer Space Telescope, we have obtained 3.6--24 micron photometry
of 38 radio galaxies and 24 quasars from the 3CR catalog at redshift 1<z<2.5.
This 178 MHz-selected sample is unbiased with respect to orientation and
therefore suited to study orientation-dependent effects in the most powerful
active galactic nuclei (AGN). Quasar and radio galaxy subsamples matched in
isotropic radio luminosity are compared. The quasars all have similar spectral
energy distributions (SEDs), nearly constant in nu F_nu through the rest 1.6-10
micron range, consistent with a centrally heated dust distribution which
outshines the host galaxy contribution. The radio galaxy SEDs show larger
dispersion, but the mean radio galaxy SED declines from rest 1.6 to 3 micron
and then rises from 3 to 8 micron. The radio galaxies are on average a factor
3-10 less luminous in this spectral range than the quasars. These
characteristics are consistent with composite emission from a heavily reddened
AGN plus starlight from the host galaxy. The mid-infrared colors and radio to
mid-infrared spectral slopes of individual galaxies are also consistent with
this picture. Individual galaxies show different amounts of extinction and host
galaxy starlight, consistent with the orientation-dependent unified scheme.
