- Conference date: 9–12 March 2009
- Location: Kailua‐Kona (Hawaii)
We discuss the application of near‐infrared (NIR) radial velocity (RV) searches for detecting planets around the lowest‐mass stars. We summerize the current methods applied to measure precise radial velocities at the m/s level in the optical, and outline the criteria for extending these methods into the near‐infrared to achieve similar performance at longer wavelengths.
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