Image Details

Choose export citation format:

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 15.

Kiel diagrams (Teff vs. ﹩\mathrm{log}g﹩) for six representative open clusters, demonstrating the physical fidelity of the derived parameters. The light-gray background points represent the entire cluster membership, derived specifically from the Gaia DR3 GSP-Phot PHOENIX library to avoid artificial discontinuities, visualizing the complete evolutionary structure. The overlaid colored points represent the high-fidelity subsample derived from our BMA model, color coded by the predicted metallicity ([M/H]). This visualization explicitly highlights the deliberate truncation of the warm upper main sequence (Teff ≳ 5800 K). The solid red curves represent the best-matching PARSEC theoretical isochrones, anchored by literature age priors (logAge) and dynamically scaled by our model’s median predicted metallicity (derived Z). The inset panels provide a zoomed-in view of the 4000–6000 K regime, confirming that our model’s predictions robustly reconstruct well-defined lower main sequences and red clump features that naturally align with theoretical evolutionary tracks.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse