Free Access
Volume 575, March 2015
Article Number A119
Number of page(s) 19
Section Planets and planetary systems
Published online 06 March 2015

Online material

Appendix A: RVs

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.

Table A.1

GJ 3293 RVs, their uncertainty and activity indicators.

Table A.2

GJ 3341 RVs, its uncertainty and activity indicators.

Table A.3

GJ 3543 RVs, its uncertainty and activity indicators.

© ESO, 2015

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