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Stellar Parameters and Chemical Abundances for 20,032 Open Cluster Members from Gaia XP Spectra Using a Boosting Multihead Attention Network

  • Authors: Jingzhen Sun, Yude Bu, Jiangchuan Zhang, Mengmeng Zhang, ShanShan Li, Yuhang Zhang, Ke Wang, Zhenping Yi, Xiaoming Kong, Meng Liu, Minglei Wu

Jingzhen Sun et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 8.

Calibration curves comparing the predicted uncertainty (σpred, x-axis) with the observed rms error (y-axis). The orange points represent the observed error after correcting for the intrinsic APOGEE label uncertainty. The dashed line indicates perfect calibration (y = x). Points on the line indicate accurate calibration (e.g., Teff). Points below the line (e.g., high-uncertainty ﹩\mathrm{log}g﹩) indicate conservative/overestimated uncertainty. Points above the line (e.g., high-uncertainty abundances) indicate overconfidence/underestimated uncertainty. The specific behavior of ﹩\mathrm{log}g﹩ at the high end is associated with the main-sequence population.

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