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A General-Purpose VLM Can Teach an Astronomy Foundation Model to Better Recognize Galaxy Morphology

Authors

Do you know Dichang Zhang?You can claim authorship or link another user.Do you know Jiaqi Deng?You can claim authorship or link another user.Do you know Yixuan Shao?You can claim authorship or link another user.Do you know Yuanpeng Liu?You can claim authorship or link another user.Do you know Jiali Cui?You can claim authorship or link another user.Do you know Zhiqiang Lao?You can claim authorship or link another user.Do you know Heather Yu?You can claim authorship or link another user.Do you know Liang Peng?You can claim authorship or link another user.Do you know Simon Birrer?You can claim authorship or link another user.Do you know Dimitris Samaras?You can claim authorship or link another user.

Abstract

Existing astronomy foundation models provide strong galaxy representations, but adapting them to new survey conditions and survey-specific morphology recognition tasks still requires substantial human supervision. We show that VLM-based VQA systems contain meaningful visual-semantic priors that can serve as weak supervision for downstream morphology classifiers and improve morphology classification under limited human-label budgets. We first introduce a survey-oriented VQA benchmark spanning two representative imaging regimes and evaluate state-of-the-art VLMs on galaxy morphology questions. The results show that these models capture useful morphology signals and informative uncertainty, but are not sufficiently reliable to replace human annotators. Motivated by this finding, we use a general-purpose VLM as a morphology teacher for Zoobot, an astronomy foundation model pretrained on large-scale Galaxy Zoo annotations. Across two survey domains and multiple annotation budgets, the VLM teacher consistently improves Zoobot's downstream morphology classification. These results demonstrate that a general-purpose VLM provides knowledge complementary to an astronomy foundation model and can teach it to better recognize galaxy morphology under limited human supervision. The resulting pipeline is designed for label-efficient adaptation to forthcoming large-scale surveys, including the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) and the Nancy Grace Roman Space Telescope. The benchmark and code are publicly available at https://github.com/fw-ic/VLM-morphology-teacher.

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Publication notes

Author note
12 pages, 5 figures