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Caption: Figure 1.
Broadband light curves data/models, systematic-removed phase curves, and residuals for the Eureka! (v1) data reductions. While NRS1 data demonstrated a significant ramp for both v1 and v2 datasets, systematic models were able to compensate and fit light-curve data adequately. Details for the orbital and system parameters used in the light-curve models are shared in Table A1. The reduced ﹩{\chi }_{\nu }^{2}﹩ and scatter multiplier (κscatter) are provided as metrics of the model fit quality and the required error inflation for each white light curve.
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