The GAPS Programme at TNG - XXXVI. Measurement of the Rossiter-McLaughlin effect and revising the physical and orbital parameters of the HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, HAT-P-29 eccentric planetary systems

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Fig. 5

RV data of the transit of HAT-P-29 b observed with HARPS-N (this work). Left-hand panels: the red line represents the best-fitting model of the RM effect; the RV residuals are plotted in the lower panel. Right-hand panels: same as left panels but with the RM effect and CB effect modelled simultaneously (green-dashed line).

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