Corner plots of modelled parameters obtained from sampling the transit light curves of TOI-1268 b. The first four columns from the left (r, i, u₁, u₂) are parameters are uniform for the whole modelled segment of transit light curves. The fifth column gives the variance of the excess white noise in the observations. The last five columns (t_c, A, t_in, t_out, σ_DR) show parameters obtained from sampling transit 3 of the planet, which had decisive evidence for one spot occultation event.