Re-evaluating the Very Hot Gas Giant WASP-12b
Re-evaluating the Very Hot Gas Giant WASP-12b
Re-evaluating the Very Hot Gas Giant WASP-12b
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Planet/Star Flux Density (10 -3 )<br />
More physically motivated models<br />
do not significantly improve <strong>the</strong> fit.<br />
z J H K 3.6 4.5 5.8 8.0<br />
A high C/O ratio cannot be defended<br />
when a two-parameter (blackbody) model fits as well<br />
as many-parameter (radiative-transfer) models.<br />
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