Fig. 2
Phase folded radial velocities of WASP−113 (left) and WASP-114 (right). The observations taken with SOPHIE are plotted as circles and those taken with CORALIE as squares. The overplotted black curve is the most probable fit orbital model and the residuals from these fits are also given (bottom panel). For WASP-113b we impose a circular orbit, while the eccentricity was left free in the model of WASP-114b.
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