WFC3 and Spitzer IRAC eclipse depths fit with the two different toy models. The black points are the WFC3 and Spitzer points. The water band points (in blue) are omitted from the fits. Photometric eclipse depths in different bands are shown but are not incorporated in this fit, following Stevenson et al. (2014, 2017). The reflected light plus thermal emission model is strongly preferred over the thermal-only model (ΔBIC = 277).