Absolute corrected carbon abundance A(C)_corr against metallicity [Fe/H], corrected for evolutionary effects from corrections by V. M. Placco et al. (2014). The Yoon–Beers taxonomy for CEMP-no progenitors is shown with blue, green, and orange ellipses (J. Yoon et al. 2016; Y. S. Lee et al. 2025). A new CEMP star is marked in magenta, and previously identified CEMP stars that are part of our targets are highlighted. All our reported CEMP stars are CEMP-no stars and reside in the Group II taxonomy.