, and [Fe/H] estimates are in good agreement with those in the DESI EDR catalog, except for The reality that a minor portion of stars from the latter experience synthetic grid consequences. For spectra with S/N > 20, the discrepancies show an Total dispersion of ∼sixty K in T The https://billionairebrainwaverevie20739.getblogs.net/65311200/examine-this-report-on-the-stellar-abundance-review