Fig. 3.
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Rotational light curve of comet 3I/ATLAS phased with a spin period of 16.16 ± 0.01 h. Photometric data points from multiple telescopes are shown with error bars; their MPC codes are listed in the box within the figure. The red solid line represents the best-fitting second-order Fourier model to the phased light curve. The MPC codes correspond to the following telescopes: C65 (Telescopi Joan Oró), E10 (FTS), F65 (FTN), M28 (Lesedi telescope), and Z23 (NTO).
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