Fig. 5
Location of WASP-78b and WASP-79b in the exoplanet equilibrium temperature-radius diagram. The filled-circles are the non-main sequence constrained parameters, while the filled-square gives the main-sequence constrained parameters for WASP-79b. The open circles shows the values obtained using the stellar radii inferred from the spectroscopic log g values (see text for discussion). Values for other exoplanets were taken from TEPCAT (Southworth 2009).
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