An extrasolar planetary system with three Neptune-mass planets

doi:doi:10.1038/nature04828

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An extrasolar planetary system with three Neptune-mass planets

Christophe Lovis, Michel Mayor, Francesco Pepe, Yann Alibert, Willy Benz, François Bouchy, Alexandre C. M. Correia, Jacques Laskar, Christoph Mordasini, Didier Queloz, Nuno C. Santos, Stéphane Udry, Jean-Loup Bertaux & Jean-Pierre Sivan

Nature 441, 305-309(18 May 2006)

doi:10.1038/nature04828

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Supplementary Table 1

This table contains the 74 radial velocity measurements of the star HD 69830 that we have obtained with the HARPS instrument. The format is ASCII text with a tabulation as separation character. The first column contains the epoch of the measurements as Barycentric Julian Date (BJD) minus 2,400,000 (for clarity). The second column gives the radial velocity of the star in km s^-1 relative to the Solar System barycenter. Finally, the third column gives the uncertainties on the measurements in km s^-1.

Supplementary Table 1 - Download Text file (2KB)

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