Photometric evolution of SN 2019odp in the ugriz′J bands using the combined photometry dataset. The colour denotes the band and the different markers denote the source instrument. The faintly overlaid light curves are light curve realisations drawn from the conditioned Gaussian process interpolation kernel (see Sect. 2.4 for a detailed description). The light curves have not been corrected for extinction. The times of spectroscopic observations are marked in the top bar by vertical lines.