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Precise Infrared Radial Velocities from Keck/NIRSPEC and the Search for Young Planets

ASTROPHYSICAL JOURNAL, no. 1 (2012): 16

Cited by: 61|Views3

Abstract

We present a high-precision infrared radial velocity (RV) study of late-type stars using spectra obtained with NIRSPEC at the W. M. Keck Observatory. RV precisions of 50 m s(-1) are achieved for old field mid-M dwarfs using telluric features for wavelength calibration. Using this technique, 20 young stars in the beta Pic (age similar to 1...More

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