, and [Fe/H] estimates are in great settlement with These during the DESI EDR catalog, except for The point that a minimal part of stars from the latter have problems with artificial grid outcomes. For spectra with S/N > 20, the dissimilarities exhibit an overall dispersion of ∼sixty K in https://rylanwqgxo.slypage.com/33278128/what-does-the-stellar-abundance-mean