Towards Galaxy Foundation Models with Hybrid Contrastive Learning
Not on the map. Why?
Abstract (arXiv)
New astronomical tasks are often related to earlier tasks for which labels have already been collected. We adapt the contrastive framework BYOL to leverage those labels as a pretraining task while also enforcing augmentation invariance. For large-scale pretraining, we introduce GZ-Evo v0.1, a set of 96.5M volunteer responses for 552k galaxy images plus a further 1.34M comparable unlabelled galaxies. Most of the 206 GZ-Evo answers are unknown for any given galaxy, and so our pretraining task uses a Dirichlet loss that naturally handles unknown answers. GZ-Evo pretraining, with or without hybrid learning, improves on direct training even with plentiful downstream labels (+4% accuracy with 44k labels). Our hybrid pretraining/contrastive method further improves downstream accuracy vs. pretraining or contrastive learning, especially in the low-label transfer regime (+6% accuracy with 750 labels).
Key facts. Cited by 10 papers in the map (data through 14 Oct 2026). Builds on 16 of its 28 references that are in the map. First posted on arXiv 23 Jun 2022.
Builds on
16 of 28 references.
References · 16
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4 more
- 2015Rotation-invariant convolutional neural networks for galaxy morphology predictioncited by 83
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Built on by
Citing papers per year: 2022: 1; 2023: 5; 2024: 3; 2025: 1.
10 papers.
- 2024Masked Particle Modeling on Sets: Towards Self-Supervised High Energy Physics Foundation Modelscited by 46
- 2024Re-Simulation-based Self-Supervised Learning for Pre-Training Foundation Modelscited by 22
- 2022Astronomia ex machina: a history, primer, and outlook on neural networks in astronomycited by 17
- 2023DeepAstroUDA: Semi-Supervised Universal Domain Adaptation for Cross-Survey Galaxy Morphology Classification and Anomaly Detectioncited by 8
- 2023A brief review of contrastive learning applied to astrophysicscited by 5
- 2024Scaling Laws for Galaxy Imagescited by 5
- 2025Are vision language models robust to uncertain inputs?cited by 3
- 2023AstroCLIP: A Cross-Modal Foundation Model for Galaxiescited by 1
- 2023Rare Galaxy Classes Identified In Foundation Model Representationscited by 1
- 2023Deep Learning Segmentation of Spiral Arms and Barscited by 0
- 2025Are vision language models robust to uncertain inputs?17 May 2025
- 2024Scaling Laws for Galaxy Images3 Apr 2024
- 2024Re-Simulation-based Self-Supervised Learning for Pre-Training Foundation Models11 Mar 2024
- 2024Masked Particle Modeling on Sets: Towards Self-Supervised High Energy Physics Foundation Models24 Jan 2024
- 2023Rare Galaxy Classes Identified In Foundation Model Representations5 Dec 2023
- 2023Deep Learning Segmentation of Spiral Arms and Bars5 Dec 2023
- 2023AstroCLIP: A Cross-Modal Foundation Model for Galaxies4 Oct 2023
- 2023A brief review of contrastive learning applied to astrophysics8 Jun 2023
- 2023DeepAstroUDA: Semi-Supervised Universal Domain Adaptation for Cross-Survey Galaxy Morphology Classification and Anomaly Detection3 Feb 2023
- 2022Astronomia ex machina: a history, primer, and outlook on neural networks in astronomy7 Nov 2022