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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 5.

Residual distributions of the stellar labels estimated by the model on the test set. The residuals are defined as ΔX = Xpred − Xlabel, where Xlabel refers to the APOGEE reference values. In each panel, the gray histogram displays the density distribution of the residuals, and the solid red curve represents the best-fit Gaussian profile. The vertical dashed line marks the position of zero bias. The statistical metrics, including the mean bias (μ) and the standard deviation (σ, representing the prediction precision), are annotated in the top-left corner of each panel.

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