Comparison between our composite TP profile (black) with those published in the literature retrieved from secondary eclipse observations by Borsa et al. (2022, red), Yan et al. (2022, blue), and Fu et al. (2022, green). As a further comparison, the dashed green line shows the result of the forward model presented by Fu et al. (2022). We recall that the retrieved profiles are an average over the illuminated planet disk; the black line is computed for the sub-stellar point.