Flow chart of CNN. Gaia-RVS spectra are used as input spectra and passed through the convolution layers for feature extraction. Extra information is fed to the CNN in the form of Gaia DR3 parallaxes as well as G, G_BP, and G_RP photometry (on the left) and XP coefficients (on the right). The information is fully connected (FC) to the output labels T_eff, log(g), [M/H], [α/M], and [Fe/H].