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Fig. 10

image

WASP-151b, WASP-153b and WASP-156b in the radius versus orbital period (left) and the mass versus orbital period (right) domains. The colored points correspond to the known exoplanet and the color reflect their bolometric incident flux. WASP-151b, WASP-153b and WASP-156b are circled in black and the black dashed lines correspond to the upper and lower boundaries of the Neptunian desert as reported by Mazeh et al. (2016), see Sect. 4.4for details.

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