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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 13.

Average normalized spectra of the VMP candidates, grouped by effective temperature (Teff). The black lines represent the “known VMP” reference sample (including literature crossmatches and DESI pipeline VMPs), while the red lines represent the “newly discovered VMP” candidates identified solely by our deep learning framework. The left column displays the full wavelength range, and the right column shows a zoomed-in view of the metallicity-sensitive Ca II K and H region (3850–4050 Å). Solid lines indicate the average flux of the respective samples, with the shaded regions indicating the 1σ dispersion.

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