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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 7.

The dependence of the model-predicted uncertainty on the stellar parameters for the test set. The background gray hexbins display the number density of stars on a logarithmic scale. The red solid line with markers represents the median predicted uncertainty calculated in 20 equidistant bins across the parameter range. The red shaded region indicates the 68% interquartile range (16th–84th percentiles) of the uncertainty distribution within each bin.

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