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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 1.

Comparison of the parameter space distributions between the training dataset (APOGEE labels) and the application dataset (open cluster members). Left panels: color–magnitude diagrams showing the domain coverage (MG vs. GBP − GRP). The background gray points represent the entire sample of quality-filtered open cluster candidates. The overlaid density contours (logarithmic scale) display the distribution of the final matched application set (top) and the training set (bottom). Middle panels: Kiel diagrams (﹩\mathrm{log}g﹩ vs. Teff) illustrating the physical parameter distribution. The points are color-coded by their metallicity ([M/H]). The top panel shows the matched open cluster members, while the bottom panel depicts the training sample. Right panels: normalized one-dimensional distribution comparisons for effective temperature (Teff), surface gravity (﹩\mathrm{log}g﹩), and metallicity ([M/H]). The blue shaded histograms represent the final matched application set, while the red dashed lines represent the training dataset.

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