, and [Fe/H] estimates are in fantastic agreement with Individuals within the DESI EDR catalog, apart from The reality that a small part of stars in the latter suffer from synthetic grid outcomes. For spectra with S/N > twenty, the variations show an In general dispersion of ∼60 K in https://billionairebrainwaverevie05668.blogofoto.com/63921124/facts-about-the-stellar-abundance-revealed