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. 4

RV data of the transit of HAT-P-26 b observed with HARPS-N (this work). Superimposed is the best-fitting RV-curve model without the CB effect (red line). The corresponding residuals are plotted in the lower panel.

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