, and [Fe/H] estimates are in superior settlement with Individuals within the DESI EDR catalog, except for The point that a insignificant portion of stars in the latter have problems with artificial grid results. For spectra with S/N > 20, the differences exhibit an In general dispersion of ∼sixty K https://collinpbejn.webdesign96.com/33265844/the-stellar-abundance-review-options