  We present a possible NASA key project using the iSHELL near-infrared
high-resolution echelle spectrograph on the NASA Infrared Telescope Facility
for precise radial velocity follow-up of candidate transiting exoplanets
identified by the NASA TESS mission. We briefly review key motivations and
challenges with near-infrared radial velocities. We present the current status
of our preliminary radial velocity analysis from the first year on sky with
iSHELL.
