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Galaxy Morphological Classification with Efficient Vision Transformer

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arxiv 2110.01024 v2 pith:PJHRW5TW submitted 2021-10-03 astro-ph.GA

classification astro-ph.GA
keywords galaxybeenclassificationgalaxiescnnsimportantmorphologicalmorphology
verification ladder T0 review T1 audit T2 compute T3 formal
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Quantifying the morphology of galaxies has been an important task in astrophysics to understand the formation and evolution of galaxies. In recent years, the data size has been dramatically increasing due to several on-going and upcoming surveys. Labeling and identifying interesting objects for further investigations has been explored by citizen science through the Galaxy Zoo Project and by machine learning in particular with the convolutional neural networks (CNNs). In this work, we explore the usage of Vision Transformer (ViT) for galaxy morphology classification for the first time. We show that ViT could reach competitive results compared with CNNs, and is specifically good at classifying smaller-sized and fainter galaxies. With this promising preliminary result, we believe the ViT network architecture can be an important tool for galaxy morphological classification for the next generation surveys. Our open source, is publicly available at \url{https://github.com/sliao-mi-luku/Galaxy-Zoo-Classification}

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. ViT-based Local Volume dwarf galaxy Identificationin (VIDA) in the CSST survey

    astro-ph.GA 2025-06 conditional novelty 6.0 of 10

    A Vision Transformer trained on simulated CSST images identifies Local Volume dwarf galaxies with 85% true positives at 0.1% false positives, reaching M_V = -7 within 10 Mpc.

  2. Capturing star formation activity from compressed photometric images of galaxies

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    A Vision Transformer trained on SDSS JPEG composites distinguishes star-forming galaxies from passive ones with about 86% accuracy and predicts BPT line ratios.

  3. GraViT: Transfer Learning with Vision Transformers and MLP-Mixer for Strong Gravitational Lens Discovery

    cs.CV 2025-08 conditional novelty 4.0 of 10

    Fine-tuned Vision Transformers and MLP-Mixer models reach lens-detection accuracy comparable to convolutional baselines on the common test sample from More et al. (2024).

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