Fig. 1.
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Number of sources per class, sorted in decreasing order. The bars shaded in yellow correspond to variability types published in the vari_classifier_result table, while galaxies, identified by their artificial photometric variations in Gaia, are published exclusively in galaxy_candidates. The ACV|CP|MCP|ROAM|ROAP|SXARI class group is abbreviated as ACV|CP|...|SXARI.
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