Finetuning Stellar Spectra Foundation Models with LoRA

Fuente: arXiv
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Main Authors: Zhao, Xiaosheng, Ting, Yuan-Sen, Szalay, Alexander S., Huang, Yang
Format: Preprint
Published: 2025
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author Zhao, Xiaosheng
Ting, Yuan-Sen
Szalay, Alexander S.
Huang, Yang
author_facet Zhao, Xiaosheng
Ting, Yuan-Sen
Szalay, Alexander S.
Huang, Yang
contents Foundation models are beginning to impact stellar spectroscopy, where spectra encode rich physical information in a structured, language-like form. A key challenge is adapting these models across heterogeneous surveys with differing resolution and coverage. We apply Low-Rank Adaptation (LoRA) to fine-tune SpecCLIP--a contrastively pre-trained model on LAMOST and Gaia XP spectra--for downstream tasks on DESI Early Data Release (EDR) spectra. We show that LoRA enables few-shot learning on DESI, with performance varying by fine-tuned module and benefiting from Gaia XP knowledge embedded in the pre-trained model. Our results demonstrate that LoRA provides a lightweight and effective strategy for extending spectral foundation models to new instruments and survey domains.
format Preprint
id arxiv_https___arxiv_org_abs_2507_20972
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Finetuning Stellar Spectra Foundation Models with LoRA
Zhao, Xiaosheng
Ting, Yuan-Sen
Szalay, Alexander S.
Huang, Yang
Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
Foundation models are beginning to impact stellar spectroscopy, where spectra encode rich physical information in a structured, language-like form. A key challenge is adapting these models across heterogeneous surveys with differing resolution and coverage. We apply Low-Rank Adaptation (LoRA) to fine-tune SpecCLIP--a contrastively pre-trained model on LAMOST and Gaia XP spectra--for downstream tasks on DESI Early Data Release (EDR) spectra. We show that LoRA enables few-shot learning on DESI, with performance varying by fine-tuned module and benefiting from Gaia XP knowledge embedded in the pre-trained model. Our results demonstrate that LoRA provides a lightweight and effective strategy for extending spectral foundation models to new instruments and survey domains.
title Finetuning Stellar Spectra Foundation Models with LoRA
topic Instrumentation and Methods for Astrophysics
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2507.20972