Comparison of the evolution of the absolute light curves in g/V (panel A, left) and r/R (panel B, middle) bands between SN 2019odp and selected comparison objects. In addition, the pseudo-bolometric light curve derived using the Lyman method is shown (panel C, right). In the pseudo-bolometric light curve (panel C), the error bars around the peak represent the combined error from the distance uncertainty, extinction uncertainty, and the scatter from the Lyman relation. The interpolated light curves for each supernova have been placed over the observed datapoints in the same colour. These were used to derive the pseudo-bolometric light curves in the right panel. The bottom left corners of panels A and B zoom in on the very early evolution.