Corner plot of the joint-fit of aperture extracted light curves with GPs. The eclipse depth f_p/f_* can be seen to be slightly correlated with many of the parameters which describe the baseline flux or detector settling in each eclipse. The slope in baseline flux is also somewhat degenerate with the initial detector settling slope for each eclipse. For many of the hyperparameters a log-uniform prior was used and so the logarithm of these parameters is plotted. Note the unusual relationship between the two eccentricity parameters which is explained in Appendix C.