, and [Fe/H] estimates are in great agreement with People within the DESI EDR catalog, except for The point that a minimal part of stars within the latter suffer from synthetic grid outcomes. For spectra with S/N > 20, the differences exhibit an overall dispersion of ∼60 K in T https://billionaire-brain-wave-re83825.blogdon.net/how-much-you-need-to-expect-you-ll-pay-for-a-good-the-stellar-abundance-review-48872905