Search for radial velocity variations in eight M-dwarfs with NIRSPEC/Keck II
Florian Rodler, Rohit Deshpande, Maria Rosa Zapatero Osorio, Eduardo, L. Martin, Michele M. Montgomery, Carlos del Burgo, Orlagh L. Creevey

TL;DR
This study used near-infrared spectra from NIRSPEC/Keck II to search for radial velocity variations in eight late M-dwarfs, finding no evidence of companions and highlighting instrumental effects on RV measurements.
Contribution
First application of NIRSPEC at Keck II to search for short-period companions around late M-dwarfs in the J-band, demonstrating RV precision and instrumental effects.
Findings
No RV variations detected in the sample.
RV precision achieved was 180-300 m/s.
Instrumental profile asymmetries affected previous RV measurements.
Abstract
Context. Radial velocity (RV) measurements from near-infrared spectra have become a potentially powerful tool to search for planets around cool stars and sub-stellar objects. As part of a large survey to characterize M-dwarfs using NIRSPEC at Keck II, we obtained spectra of eight late M-dwarfs (spectral types M5.0-M8.0) during two or more observing epochs per target. These spectra were taken with intermediate spectral resolving powers (R \sim 20,000) in the J-band. Aims. We search for relative radial velocity variability in these late M-dwarfs and test the NIRSPEC capability of detecting short period brown dwarf and massive planetary companions around low-mass stars in the J-band (\approx 1.25 micron). Additionally, we reanalyzed the data of the M8-type star vB10 (one of our targets) presented in Zapatero Osorio et al. (2009), which were obtained with the same instrumentation as our…
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