Stacked histograms showing the distribution of GALAH derived M 2 in the NCE and RCE samples derived from (a) GALAH DR3 parameters (this work) and (b) Gaia DR3 parameters (S. Shahaf et al. 2024). More than 50% of stars with M 2 ≈ 0.6 M ⊙ formerly classified as RCE get reclassified as NCE systems.