Fig. A.1

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Phased light curve of 2023 DZ2 computed using photometric measurements obtained within the Pro-Am collaboration discussed in the text. The title of each panel highlights the observatory (including the MPC code). The reported period and amplitude were computed by the observers using Tycho Tracker (for L04 and 073), and MPO Canopus (for Z95). The plots were made with GNU Octave software (Eaton et al. 2021), and a splinefit function was used to fit the data. In the case of 073, a binning of nine points was made after folding the photometric data.
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