Fig. 2

Radial velocity variations and line bisectors (Vspan) of WASP-78 and WASP-79 folded on the best-fitting circular orbit periods (solid lines). The eccentric orbit solutions are shown as dashed-lines (see Sect. 6 for discussion). The bisector uncertainties of twice the RV uncertainties have been adopted. The mean values of the bisectors are indicated by the dotted lines. There is negligible correlation between Vspan and orbital phase.
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