  Precision radial velocity data for HD 208487 has been re-analyzed using a new
Bayesian multi-planet Kepler periodogram. The periodgram employs a parallel
tempering Markov chain Monte Carlo algorithm with a novel statistical control
system. We confirm the previously reported orbit (Tinney et al. 2005) of 130
days. In addition, we conclude there is strong evidence for a second planet
with a period of 998 -62 +57 days, an eccentricity of 0.19 -0.18 +0.05, and an
M sin i = 0.46 -0.13 +0.05 of Jupiter's mass.
