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A Catalog of High-confidence Very Metal-poor Stars from DESI Based on a Deep Learning Method

  • Authors: Chen Yang, 晨 杨, Guanhong Lin, 观泓 林, Lei Tan, 磊 谈, Huanbin Chi, 焕斌 迟, Feng Wang, 锋 王, Hui Deng, 辉 邓, Ying Mei, 盈 梅

Chen Yang et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 12.

Corner plot of metallicity estimates for the crossmatched VMP subsample (∼500 stars). Diagonal panels show the one-dimensional distributions of [Fe/H]RVS and [Fe/H]SP from the DESI RVS and SP pipelines, the metallicity [Fe/H]GaiaXP derived by L. Yang et al. (2025) from Gaia XP spectra, and the model-predicted [Fe/H]model, with the median and 16th/84th percentiles indicated in the panel titles. Off-diagonal panels display the corresponding two-dimensional distributions for each pair of metallicity estimates.

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