The temperature-pressure (T-P) profile for the our atmospheric models used for modelling the secondary eclipse depth. The black (solid) line shows the uninverted model from Fortney et al. (2008), the green (dashed-triple dotted) line is for a model with an ad hoc temperature inversion as in Todorov et al. (2010), the red (dashed) line shows the temperature pressure profile for an atmosphere with a normal troposphere and an inversion, and the orange (dash-dotted) line is for an atmosphere with Venus-like clouds. The temperatures for the latter profiles are chosen to provide a reasonable fit to the IRAC bands longward of 4 μm.