Example of a flare fit with a well-determined width (t₀), radial separation (r₀), and inclination (ϕ). We plot the average of 100 model light curves drawn from the posterior. To make all model components comparable, the fluxes have been normalized. The light yellow line shows the averaged relativistic kernel, dark brown shows the averaged Gaussian flare kernel, dark green shows the composite model without the Gaussian process component, and light green shows the 100 realizations of the full model.