Volume 575, March 2015
|Number of page(s)||19|
|Section||Planets and planetary systems|
|Published online||06 March 2015|
The RVs are in the barycentric frame and are corrected for secular acceleration. The RVs were extracted through χ2 matching to a template with a high S/N. The errors combine the estimated photon noise with the an estimate of the residual instrumental error (0.60 m s-1). We also tabulate the FWHM and bisector span (BIS) of the CCF, as well as the activity indices of Hα and Ca II from Mount Wilson S.
GJ 3293 RVs, their uncertainty and activity indicators.
GJ 3341 RVs, its uncertainty and activity indicators.
GJ 3543 RVs, its uncertainty and activity indicators.
© ESO, 2015
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