We describe the program for detection and characterization of extra-solar
planets using the Advanced Fiber Optic Echelle (AFOE) spectrograph, developed
at Mt. Hopkins Observatory jointly by CfA and HAO. The AFOE is capable of
obtaining radial velocity precision better than 10 m s-1 on relatively bright
stars, and has produced data confirming the low mass companions to 51 Peg,
Tau Boo, and Upsilon And. We describe the current observing program for
monitoring a number of solar-like stars.