Fig. 9
Planetary radii as a function of incident flux. WASP-43 b is shown as a black square. gray filled circles are Kepler planetary candidates (see Demory & Seager 2011). Transiting giant planets previously published, and mostly from ground-based surveys, are shown as gray triangles. The relevant parameters Rp, Rs, Teff and a have been drawn from http://www.inscience.ch/transits on August 29, 2011.
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