Exoplanets around nearby M dwarfs with NIR RVs

Precise Near-Infrared Radial Velocities
http://arxiv.org/abs/1603.05999

Quote :

We present the results of two 2.3 micron near-infrared radial velocity surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ~46,000) at the NASA InfraRed Telescope Facility, combined with an isotopic methane absorption gas cell for common optical path relative 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 velocity dispersions of ~20-30 m/s on our survey targets.

They assert that they're still working on publishing the results. Doesn't look like any of the star names are in the paper.

Already some initial observations for GJ 15 A, SV Peg and GJ 876

Gao et al. (2016) "Retrieval of Precise Radial Velocities from Near-Infrared High Resolution Spectra of Low Mass Stars"
http://arxiv.org/abs/1603.05997

Also some results for over 30 stars

Gagné et al. (2016) "A High-Precision NIR Survey for RV Variable Low-Mass Stars"
http://arxiv.org/abs/1603.05998

Apparently this is the first multi-wavelength confirmation of GJ 876 b and c.

No new discoveries?

They assert that they're still working on publishing the results. Doesn't look like any of the star names are in the paper.