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FTS Measurements of Uranium Emission Lines in the Near-Infrared and their Application to the Search for Earth-Mass Exoplanets

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Abstract

Precise calibrations are needed for high-resolution near-infrared astronomical spectrographs. We have measured the wavenumbers of over 7500 uranium emission lines and used a subset of them to make precise radial velocity measurements.

© 2011 Optical Society of America

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