An abstract from the programme for the 2nd Subaru International Conference:
http://www.naoj.org/SubaruConf09/The detection of a new large mass planet orbiting around a K0 type star
Hiroki Harakawa
We report the detection of a new large mass planet orbiting around a K0 type star(V=8.26)
which has a minimum mass Msin i=8.9 Jupiter mass in a 692.9 day orbit by precise radial
velocity measurements from Subaru and Keck. The derived orbital parameters based on minimizing
chi square by down-hill simplex method suggest that these radial velocity variations
are consistent with an almost circular planet orbit and a Mars-like semimajor axis (e=0.04,
a=1.6AU). The residuals to a single-Keplerian fit suggest the possible stellar wobbling by
another companion which has lower mass and a shorter period than the primary one.
And maybe another planet in the system on the way.