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. 1

RV data of the transit of HAT-P-15 b observed with HARPS-N. Superimposed are the best-fitting RV-curve models (the red line does not include the modelling of the stellar convective blueshift (CB) effect, while the green-dashed line does). The corresponding residuals are plotted in the lower panel. For clarity, the error bars are displayed only for the model without the CB effect. See the discussion in Sect. 8.2

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