, and [Fe/H] estimates are in good agreement with those within the DESI EDR catalog, except for the fact that a insignificant portion of stars inside the latter suffer from synthetic grid effects. For spectra with S/N > twenty, the variances exhibit an overall dispersion of ∼sixty K in T https://billionairebrainwaverevie97354.blogproducer.com/39602969/what-does-the-stellar-abundance-mean