VizieR Online Data Catalog: M dwarf stars rotational broadening measurements (Kesseli+, 2018)

Data were collected between 2016 October and 2017 November using the Immersion GRating INfrared Spectrograph (IGRINS; Park et al. 2014SPIE.9147E..1DP) on Lowell Observatory's 4.3 m Discovery Channel Telescope (DCT) at and the 2.7 m Harlan J. Smith Telescope at McDonald Observatory. We also used iSHELL (Rayner et al. 2016SPIE.9908E..84R) on NASA's 3.0 m Infrared Telescope Facility (IRTF) on Mauna Kea, Hawaii. IGRINS is a high-resolution (R~45000) infrared spectrograph that simultaneously collects H and K-band spectra (Mace et al. 2016SPIE.9908E..0CM). iSHELL has a spectral resolution of 75000 at our chosen wavelength region in the K-band (2.26-2.55 μm).

(1 data file).