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Fig. 4


Synthetic emission spectra of the planets WASP-32b and WASP-10b for the clear fiducial models with solar C/O ratios and for the cases with C/O ratios twice as large as solar. We also plot existing Spitzer photometry for the targets by Garland et al. (2016, WASP-32b) and Kammer et al. (2015, WASP-10b). A dayside-averaged insolation was assumed for both planets. For clarity, both the synthetic spectra and data of WASP-32b have been multiplied by an offset factor of three.

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