  We will present the results of a NICMOS H-band imaging survey of a small
sample of z ~ 2 to 3 radio-quiet quasars. We have resolved extension in at
least 4 of 5 objects and find evidence for a wide range in the morphologies and
magnitudes of these hosts. The host galaxy luminosities range from sub-L* to
about 4 L*, with most of the hosts having luminosities about L*. These host
galaxies have magnitudes and sizes consistent with those of the Ly break
galaxies at similar redshifts and at similar rest wavelengths, but are about a
magnitude fainter than the comparable 6C radio galaxies. One residual host
component is not centered on the quasar nucleus, and several have close
companions (within ~10 kpc), indications that these systems are possibly in
some phase of a merger process.
