Noise-model-corrected transits of K2-19 d (dots with the same color code as in Fig. 2), the MAP model (black line), and the continuous oversampled MAP model (gray line) from the photodynamical modeling. Each panel is centered at the linear ephemeris (indicated by the vertical gray lines). Each panel is labeled with the telescopes that observed and the epoch number. The residuals after subtracting the MAP model are shown in the lower part of each panel.