  A NASA sounding rocket for high contrast imaging with a visible nulling
coronagraph, the Planet Imaging Coronagraphic Technology Using a Reconfigurable
Experimental Base (PICTURE-B) payload has made two suborbital attempts to
observe the warm dust disk inferred around Epsilon Eridani. We present results
from the November 2015 launch demonstrating active wavefront sensing in space
with a piezoelectric mirror stage and a micromachine deformable mirror along
with precision pointing and lightweight optics in space.
