, and [Fe/H] estimates are in good settlement with These while in the DESI EDR catalog, except for The reality that a minor percentage of stars in the latter suffer from synthetic grid results. For spectra with S/N > twenty, the distinctions exhibit an General dispersion of ∼60 K in https://billionairebrainwaverevie49370.fitnell.com/73520586/not-known-facts-about-the-stellar-abundance