Part of the latent space where the ANN projects eclipsing and ellipsoidal binaries. The grey background shows the same density as in Fig. 13. Sources that were published in the Gaia DR3 Variability catalogue gaiadr3.vari_eclipsing_binary are overplotted in a 2D histogram of small hexagons where the colour of each hexagon corresponds to the average magnitude difference between primary and secondary eclipses of the sources inside that bin.