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Paper: Detecting Planets around Very Cool Stars at Near Infrared Wavelengths with the Radial Velocity Technique
Volume: 430, Pathways Towards Habitable Planets
Page: 526
Authors: Rodler, F.; del Burgo, C.; Martín, E. L.; Álvarez, C.
Abstract: The radial velocity (RV) technique in the near-infrared is a powerful tool to search for low-mass planets around cool stars and sub-stellar objects. We investigate what precision can be achieved in RV measurements of an M9-dwarf in the Y-, J-, H-, and K-bands. Although late M-dwarfs emit the most flux in the J-band, we find that the highest RV-precision is attained in the Y-band.
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