Precision radial velocities with CSHELL
arXiv:1104.3804 · doi:10.1088/0004-637X/735/2/78
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.
31 pages, 3 figures, 2 tables, accepted for publication in ApJ
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Cited by in corpus (15)
- Metallicity and Temperature Indicators in M dwarf K band Spectra: Testing New & Updated Calibrations With Observations of 133 Solar Neighborhood M dwarfs
- A High-Precision NIR Survey for RV Variable Low-Mass Stars
- Identifying the young low-mass stars within 25 pc. II. Distances, kinematics and group membership
- SOAP. A tool for the fast computation of photometry and radial velocity induced by stellar spots
- A Candidate Young Massive Planet in Orbit around the Classical T Tauri Star CI Tau
- Precise Infrared Radial Velocities from Keck/NIRSPEC and the Search for Young Planets
- The PTF Orion Project: a Possible Planet Transiting a T-Tauri Star
- A Search for Giant Planet Companions to T Tauri Stars
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- Keck NIRSPEC Radial Velocity Observations of Late-M dwarfs
- Retrieval of Precise Radial Velocities from Near-Infrared High Resolution Spectra of Low Mass Stars
- H-alpha Variability in PTFO8-8695 and the Possible Direct Detection of Emission from a 2 Million Year Old Evaporating Hot Jupiter
- Finding proto-spectroscopic binaries: Precise multi-epoch radial velocities of 7 protostars in rho-Ophiuchus
- Multiplexing Precision RVs: Searching for Close in Gas Giants in Open Clusters