Browse State-of-the-Art › Morphology classification
Morphology classification
17 papers with code · 0 benchmarks · 0 datasets archive 2025-07-28
Benchmarks archive 2025-07-28
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Datasets archive 2025-07-28
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Parent tasks archive 2025-07-28
Most implemented papers archive 2025-07-28
17 shown of 17 papers with code (30 tagged with this task in all), ordered by repositories listed in the archive, not by stars (the archive holds no stars, so PwC's “Social” and “Latest” sorts cannot be reproduced). Papers without a page here are shown as plain text.
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8 Nov 2021 2 repositories listedThe predicted results are then used to generate accuracy metrics per decision tree question to determine architecture performance.
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24 Mar 2015 2 repositories listedUnfortunately, even this approach does not scale well enough to keep up with the increasing availability of galaxy images.
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19 Jun 2025 1 repository listedObservational astronomy relies on visual feature identification to detect critical astrophysical phenomena.
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20 Dec 2024 1 repository listedHowever, due to differences in signal-to-noise ratios and resolutions between the DECaLS images and those from BASS and MzLS (collectively referred to as BMz), a neural network trained on DECaLS images cannot be…
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6 Feb 2024 1 repository listedWe propose a new approach for sperm head morphology classification, called SHMC-Net, which uses segmentation masks of sperm heads to guide the morphology classification of sperm images.
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2 Nov 2023 1 repository listedWe propose the use of group convolutional neural network architectures (GCNNs) equivariant to the 2D Euclidean group, E(2), for the task of galaxy morphology classification by utilizing symmetries of the data present in…
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4 Oct 2023 1 repository listed Syntology ran 2 of 2 samples · 0 unverifiedThese embeddings can then be used - without any model fine-tuning - for a variety of downstream tasks including (1) accurate in-modality and cross-modality semantic similarity search, (2) photometric redshift…
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15 Mar 2023 1 repository listedWe further enhance our model by tuning the VAE network via DA using galaxies in the overlapping footprint of DECaLS and BASS+MzLS, enabling the unbiased application of our model to galaxy images in both surveys.
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3 Feb 2023 1 repository listedThis algorithm performs semi-supervised domain adaptation and can be applied to datasets with different data distributions and class overlaps.
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1 Nov 2022 1 repository listed Syntology ran 0 of 2 samples · 2 unverifiedFor the first time, we demonstrate the successful use of domain adaptation on two very different observational datasets (from SDSS and DECaLS).
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13 Jun 2022 1 repository listedTherefore, this paper implements unsupervised learning techniques to classify the Galaxy Zoo DECaLS dataset.
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25 Mar 2022 1 repository listedTo overcome these limitations, we present a semi-supervised transfer learning approach that uses a small number of labeled microscopy images for training and performs as effectively as methods trained on significantly…
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8 Nov 2021 1 repository listedIn this work, we examine the robustness of state-of-the-art semi-supervised learning (SSL) algorithms when applied to morphological classification in modern radio astronomy.
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24 Dec 2020 1 repository listedWe show that, without the need for labels, self-supervised learning recovers representations of sky survey images that are semantically useful for a variety of scientific tasks.
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31 Aug 2020 1 repository listedWe study the usage of EfficientNets and their applications to Galaxy Morphology Classification.
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10 Jul 2020 1 repository listedTo reduce the required computational costs, we apply machine learning techniques for clustering and consequent prediction of the simulated polymer blend images in conjunction with simulations.
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22 Sep 2018 1 repository listedIn this work, we studied the performance of Capsule Network, a recently introduced neural network architecture that is rotationally invariant and spatially aware, on the task of galaxy morphology classification.
Syntology lines on 2 of the papers shown; no Syntology record for the others (a paper without an arXiv id cannot be joined to the graph, and absence from the graph layer is not a recorded non-run). “Ran” means the sample executed on a synthesized fixture, not that the paper's result was reproduced. Read from the graph 2026-09-24.
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