  A periodic variation in the pulse timings of the pulsating hot subdwarf B
star CS 1246 was recently discovered via the O-C diagram and suggests the
presence of a binary companion with an orbital period of two weeks. Fits to
this phase variation, when interpreted as orbital reflex motion, imply CS 1246
orbits a barycenter 11 light-seconds away with a velocity of 16.6 km/s. Using
the Goodman spectrograph on the SOAR telescope, we decided to confirm this
hypothesis by obtaining radial velocity measurements of the system over several
months. Our spectra reveal a velocity variation with amplitude, period, and
phase in accordance with the O-C diagram predictions. This corroboration
demonstrates that the rapid pulsations of hot subdwarf B stars can be adequate
clocks for the discovery of binary companions via the pulse timing method.
