2D differential histogram comparing the flux distribution at a certain phase against the out-of-eclipse flux distribution for all long- (top) and short cadence (bottom) data. Excess flux compared to the out-of-eclipse histogram shows up as bright areas. We use 100 intensity bins and 320 phase bins of width 0.0125 such that the phase bins are 4 × oversampled. Note the excess flux around phase φ = -0.1 in the long cadence data indicating the forward scattering, which is not visible in the SC data.