An example result (T5) of our wavelength-dependent curve detrending and fitting. Left: raw target magnitude with corresponding GP systematics model, shown with 68% and 95% errors. Middle: detrended light curve in relative flux, with transit model. Each wavelength bin is labeled with their wavelength range as well. Right: residuals with corresponding standard deviation in ppm. The rest of the wavelength-dependent light curves are given in Appendix B.