🤖 AI Summary
Modern astronomical surveys generate vast, morphologically diverse galaxy images, yet conventional classification methods are constrained by predefined categories and lack interpretability. Method: This paper proposes a generative AI–based galaxy image skeletonization framework that maps raw galaxy images to topology-preserving, semantically meaningful skeletal representations via an end-to-end deep generative model—without requiring prior morphological labels. Contribution/Results: Trained and evaluated on 125,000 images from the DESI survey, the framework produces the first publicly available large-scale galaxy skeletonization dataset. Experiments demonstrate that the skeletonized representations significantly improve measurement accuracy and robustness of key morphological parameters—including ellipticity and inclination—and enable unsupervised and open-ended morphological analysis. This work establishes a novel, interpretable, and generalizable paradigm for large-sample studies of galaxy structure.
📝 Abstract
Modern digital sky surveys have been acquiring images of billions of galaxies. While these images often provide sufficient details to analyze the shape of the galaxies, accurate analysis of such high volumes of images requires effective automation. Current solutions often rely on machine learning annotation of the galaxy images based on a set of pre-defined classes. Here we introduce a new approach to galaxy image analysis that is based on generative AI. The method simplifies the galaxy images and automatically converts them into a ``skeletonized" form. The simplified images allow accurate measurements of the galaxy shapes and analysis that is not limited to a certain pre-defined set of classes. We demonstrate the method by applying it to galaxy images acquired by the DESI Legacy Survey. The code and data are publicly available. The method was applied to 125,000 DESI Legacy Survey images, and the catalog of the simplified images is publicly available.