Precise Near-Infrared Radial Velocities

We present the results of two 2.3 μm near-infrared (NIR) radial velocity(RV) surveys to detect exoplanetsaround 36 nearby and young M dwarfs. We use the CSHELL spectrograph ( R ~ 46,000) at the NASA InfraRed TelescopeFacility (IRTF), combined with an isotopic methane absorption gas cell for common optical pathrelative wavelength calibration. We have developed a sophisticated RV forward modeling code that accounts for fringing and other instrumental artifacts present in the spectra. With a spectral grasp of only 5 nm, we are able to reach long-term radial velocitydispersions of ~20–30 m s −1 on our survey targets.