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Fig. 5


Upper left: lightcurve of star 171895 relative to the 2004 observing season. Red points highlight transit epochs, also indicated by the roman numeration. Upper right: lightcurve of star 171895 relative to the 2009 observing season. Lower left, top panel: folded lightcurve. The continuous line indicates the best-fit model obtained using the Mandel & Agol (2002) algorithm, considering as properties of the host star those derived from the UVES spectroscopy. The roman numeration and the associated symbols are relative to the transit epochs shown in the upper panels. Lower left, bottom panel: observed minus model residuals. Lower right: UVES spectroscopic measurements.

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