Origin of the discrepancy in the [N/Fe]–[Fe/H] trend relative to APOGEE
Determine the cause of the observed discrepancy between the [N/Fe]–[Fe/H] abundance trend obtained from the Data-Driven Payne analysis of DESI Early Data Release spectra and the trend measured by APOGEE DR17.
References
The [N/Fe] shows slight different trend to APOGEE, with unclear reason.
                — Determining Stellar Elemental Abundances from DESI Spectra with the Data-Driven Payne
                
                (2402.06242 - Zhang et al., 9 Feb 2024) in Section 4.2 (Stellar abundances), paragraph discussing Fig. 7