Top: primary mass distribution of the candidate stars reported by ExoDNN (green). Also added for comparison are the mass distributions corresponding to the NSS Orbital* (orange), AstroSpectroSB1 (blue), and Eclipsing* binary (black) solutions from the DR3 NSS. The ExoDNN predictions show the 6% model false positive rate as downward arrows. Bottom: equivalent distributions but for metallicity of the candidates reported by ExoDNN.