arXiv:2111.04357
공식 코드 · Papers with Code
Can semi-supervised learning reduce the amount of manual labelling required for effective radio galaxy morphology classification?
원문 초록
In 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. We test whether SSL can achieve performance comparable to the current supervised state of the art when using many fewer labelled data points and if these results generalise to using truly unlabelled data. We find that although SSL provides additional regularisation, its performance degrades rapidly when using very few labels, and that using truly unlabelled data leads to a significant drop in performance.
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Can AI Dream of Unseen Galaxies? Conditional Diffusion Model for Galaxy Morphology Augmentation
A Versatile Framework for Analyzing Galaxy Image Data by Implanting Human-in-the-loop on a Large Vision Model
Morphological classification of astronomical images with limited labelling
Self-Supervised Representation Learning for Astronomical Images
Statistical Machine Learning for Astronomy -- A Textbook
Emulating compact binary population synthesis simulations with robust uncertainty quantification and model comparison: Bayesian normalizing flows
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