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Generalization from Low- to Moderate-resolution Spectra with Neural Networks for Stellar Parameter Estimation: A Case Study with DESI

  • Authors: Xiaosheng Zhao, Yuan-Sen Ting, Rosemary F.G. Wyse, Alexander S. Szalay, Yang Huang, László Dobos, Tamás Budavári, Viska Wei

Xiaosheng Zhao et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure A3.

Effect of the number of trainable parameters on [Fe/H] fine-tuning performance, comparing LoRA and residual-head strategies. The y-axis shows the coefficient of determination (R2) for [Fe/H] estimation using the full sample, metal-rich subset ([Fe/H] > −1.0), and metal-poor subset ([Fe/H] < −1.0). The number of test samples is 5539, with a fine-tuning set of 2069 stars. Annotations indicate the hidden-layer size for residual-head models (e.g., H384) and the rank for LoRA models (e.g., R128).

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