Similar to Fig. 23, but showing the brightness distribution of the sources in the dataset obtained by combining the LPV candidates resulting from the Gaia DR3 SOS and classification modules. The full set of sources in the direction of the MCs (left) or Galactic bulge (right) OGLE-III fields are shown with red lines. Blue lines correspond to sources matched with OGLE-III, while newly discovered candidates are represented by the green lines. Solid lines are limited to the sources resulting from the SOS module, and dashed lines include the output of the classification module as well. The green lines in the left panel show counts enhanced by a factor 20 for visual clarity.