The GAPS Programme with HARPS-N at TNG - VIII. Observations of the Rossiter-McLaughlin effect and characterisation of the transiting planetary systems HAT-P-36 and WASP-11/HAT-P-10

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Fig. 1

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Phase-folded RV data of a partial transit of HAT-P-36 b observed with HARPS-N. Superimposed is the best-fitting RV-curve model. The corresponding residuals are plotted in the lower panel. Phase 0 corresponds to the time of the planet passing the periastron.

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