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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 1.

Sketch of the pretraining and fine-tuning workflow. Pretraining uses normalized spectra or foundation-model spectral embeddings to predict labels: [Fe/H] from APOGEE (>−2.0), supplemented at lower metallicities by PASTEL, SAGA, and other VMP and UMP datasets; and [α/Fe] from APOGEE. The foundation model is trained on large unlabeled datasets. Fine-tuning then adapts the network using fewer labeled spectra, either from spectra or spectral embeddings, with different fine-tuning modules applied (see Section 3).

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