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- W2015577047 abstract "Radial velocity identification of extrasolar planets has historically been dominated by optical surveys. Interest in expanding exoplanet searches to M dwarfs and young stars, however, has motivated a push to improve the precision of near infrared radial velocity techniques. We present our methodology for achieving 58 m/s precision in the K band on the M0 dwarf GJ 281 using the CSHELL spectrograph at the 3-meter NASA IRTF. We also demonstrate our ability to recover the known 4 Mjup exoplanet Gl 86 b and discuss the implications for success in detecting planets around 1-3 Myr old T Tauri stars." @default.
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- W2015577047 date "2011-06-20" @default.
- W2015577047 modified "2023-10-18" @default.
- W2015577047 title "PRECISION RADIAL VELOCITIES WITH CSHELL" @default.
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- W2015577047 doi "https://doi.org/10.1088/0004-637x/735/2/78" @default.
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