, and [Fe/H] estimates are in fantastic arrangement with These during the DESI EDR catalog, apart from The reality that a minimal percentage of stars inside the latter experience artificial grid results. For spectra with S/N > 20, the discrepancies exhibit an overall dispersion of ∼60 K in T The https://caidenfcvog.blogitright.com/32838487/the-stellar-abundance-review-an-overview