  We present a direct image of the innermost companion to the red giant delta
Andromedae using the Stellar Double Coronagraph at the Palomar Observatory. We
use a Markov chain Monte Carlo based algorithm to simultaneously reduce the
data and perform astrometry and photometry of the companion. We determine that
the companion is most likely a main-sequence K-type star and is certainly not
the previously hypothesized white dwarf.
