This observing run was an attempt to resolve the radial veolcity variations in the star Tau Bootes caused by its extrasolar planet. We are very happy to announce that we have successfully resolved the orbit and have data analysis from two independent sources. The graph above shows our data phased over the sine wave of the planet's orbit as published by Marcy and Butler. See Tau Boo for further info.
Spectroscopy is a small field.
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