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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 13.

Cross-survey validation of fundamental parameters. Top panels: comparison against the GALAH survey (L. Spina et al. 2022) for 280 common stars. Bottom panels: comparison against the GES (L. Magrini et al. 2017) for 37 common stars. The red dashed line indicates the identity relation (y = x). The dotted lines represent the ±1σ, ±2σ, and ±3σ dispersion intervals. The top marginal panels show the probability density distributions of the optical surveys (blue) and ours (orange).

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