All occultation light curves of the unpublished stellar occultations. They are ordered by decreasing diameter of the occulting object, as in Table 1. The graphs present on the x-axis the time in seconds after midnight of the occultation date. On the y-axis, they show the relative flux, normalized to unity, of the occulted star divided by the reference stars. Some light curves were offset on the y-axis by an integer value for visualization purposes. Black lines represent the data, blue lines the model of a body without atmosphere occulting a punctual star at the derived times, and the red lines show the complete model where the Fresnel diffraction and the stellar diameter are convoluted to each finite exposure time.