A Versatile Framework for Analyzing Galaxy Image Data by Implanting Human-in-the-loop on a Large Vision Model
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| Main Authors: | , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866913354453352448 |
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| author | Fu, Mingxiang Song, Yu Lv, Jiameng Cao, Liang Jia, Peng Li, Nan Li, Xiangru Liu, Jifeng Luo, A-Li Qiu, Bo Shen, Shiyin Tu, Liangping Wang, Lili Wei, Shoulin Yang, Haifeng Yi, Zhenping Zou, Zhiqiang |
| author_facet | Fu, Mingxiang Song, Yu Lv, Jiameng Cao, Liang Jia, Peng Li, Nan Li, Xiangru Liu, Jifeng Luo, A-Li Qiu, Bo Shen, Shiyin Tu, Liangping Wang, Lili Wei, Shoulin Yang, Haifeng Yi, Zhenping Zou, Zhiqiang |
| contents | The exponential growth of astronomical datasets provides an unprecedented opportunity for humans to gain insight into the Universe. However, effectively analyzing this vast amount of data poses a significant challenge. Astronomers are turning to deep learning techniques to address this, but the methods are limited by their specific training sets, leading to considerable duplicate workloads too. Hence, as an example to present how to overcome the issue, we built a framework for general analysis of galaxy images, based on a large vision model (LVM) plus downstream tasks (DST), including galaxy morphological classification, image restoration, object detection, parameter extraction, and more. Considering the low signal-to-noise ratio of galaxy images and the imbalanced distribution of galaxy categories, we have incorporated a Human-in-the-loop (HITL) module into our large vision model, which leverages human knowledge to enhance the reliability and interpretability of processing galaxy images interactively. The proposed framework exhibits notable few-shot learning capabilities and versatile adaptability to all the abovementioned tasks on galaxy images in the DESI legacy imaging surveys. Expressly, for object detection, trained by 1000 data points, our DST upon the LVM achieves an accuracy of 96.7%, while ResNet50 plus Mask R-CNN gives an accuracy of 93.1%; for morphology classification, to obtain AUC ~0.9, LVM plus DST and HITL only requests 1/50 training sets compared to ResNet18. Expectedly, multimodal data can be integrated similarly, which opens up possibilities for conducting joint analyses with datasets spanning diverse domains in the era of multi-message astronomy. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2405_10890 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A Versatile Framework for Analyzing Galaxy Image Data by Implanting Human-in-the-loop on a Large Vision Model Fu, Mingxiang Song, Yu Lv, Jiameng Cao, Liang Jia, Peng Li, Nan Li, Xiangru Liu, Jifeng Luo, A-Li Qiu, Bo Shen, Shiyin Tu, Liangping Wang, Lili Wei, Shoulin Yang, Haifeng Yi, Zhenping Zou, Zhiqiang Instrumentation and Methods for Astrophysics Astrophysics of Galaxies Artificial Intelligence The exponential growth of astronomical datasets provides an unprecedented opportunity for humans to gain insight into the Universe. However, effectively analyzing this vast amount of data poses a significant challenge. Astronomers are turning to deep learning techniques to address this, but the methods are limited by their specific training sets, leading to considerable duplicate workloads too. Hence, as an example to present how to overcome the issue, we built a framework for general analysis of galaxy images, based on a large vision model (LVM) plus downstream tasks (DST), including galaxy morphological classification, image restoration, object detection, parameter extraction, and more. Considering the low signal-to-noise ratio of galaxy images and the imbalanced distribution of galaxy categories, we have incorporated a Human-in-the-loop (HITL) module into our large vision model, which leverages human knowledge to enhance the reliability and interpretability of processing galaxy images interactively. The proposed framework exhibits notable few-shot learning capabilities and versatile adaptability to all the abovementioned tasks on galaxy images in the DESI legacy imaging surveys. Expressly, for object detection, trained by 1000 data points, our DST upon the LVM achieves an accuracy of 96.7%, while ResNet50 plus Mask R-CNN gives an accuracy of 93.1%; for morphology classification, to obtain AUC ~0.9, LVM plus DST and HITL only requests 1/50 training sets compared to ResNet18. Expectedly, multimodal data can be integrated similarly, which opens up possibilities for conducting joint analyses with datasets spanning diverse domains in the era of multi-message astronomy. |
| title | A Versatile Framework for Analyzing Galaxy Image Data by Implanting Human-in-the-loop on a Large Vision Model |
| topic | Instrumentation and Methods for Astrophysics Astrophysics of Galaxies Artificial Intelligence |
| url | https://arxiv.org/abs/2405.10890 |