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WASP-17b: an ultra-low density planet in a probable retrograde orbit

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Fig. 2.— Upper panel: Euler I c -band light curve (red circles) taken on 2008 May 06. Overplotted are the best-fitting model transits (solid lines; §4) from the parameters of Table 4; consult that table for the key to the colour and symbol scheme
Fig. 4.— Bisector span versus relative radial velocity for the CORALIE (red circles) and HARPS (blue squares) spectra
Fig. 5.— Modified H-R diagram: inverse cube-root of stellar den- den-sity versus stellar effective temperature
Fig. 6.— Zoom-in on the spectroscopic transit region of Figure 3, showing the fitted RM effect more clearly
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