, and [Fe/H] estimates are in excellent agreement with All those from the DESI EDR catalog, aside from The truth that a insignificant percentage of stars in the latter suffer from artificial grid consequences. For spectra with S/N > twenty, the distinctions exhibit an overall dispersion of ∼sixty K in https://cristianawqiz.develop-blog.com/39540842/the-stellar-abundance-review-for-dummies