A CCD camera operating at T = 65 K was mounted in the vacuum space of
our nuclear demagnetization cryostat. This has allowed us to make obse
rvation ns of He-3 crystals at temperatures below the superfluid phase
transitions, in contrast to direct optical observations, which have s
o far been limited to T greater than or equal to 20 mK.(1) The good th
ermal equilibrium provided by the superfluid allows us to nucleate sin
gle crystals of He-3 in the region of the cell visible to the optical
system. This occurs either spontaneously (due either to gravitational
pressure gradients or focal surface defects) or as a result of a small
applied heat pulse.