Data-driven image restoration with option-driven learning for big and small astronomical image data sets
Jia, Peng ; Ning, Ruiyu ; Sun, Ruiqi ; Yang, Xiaoshan ; Cai, Dongmei
Image restoration methods are commonly used to improve the quality of astronomical images. In recent years, developments of deep neural networks and increments of the number of astronomical images have evoked a lot of data-driven image restoration methods. However, most of these methods belong to supervised learning algorithms, which require paired images either from real observations or simulated data as training set. For some applications, it is hard to get enough paired images from real observations and simulated images are quite different from real observed ones. In this paper, we propose a new data-driven image restoration method based on generative adversarial networks with option-driven learning. Our method uses several high-resolution images as references and applies different learning strategies when the number of reference images is different. For sky surveys with variable observation conditions, our method can obtain very stable image restoration results, regardless of the number of reference images.
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Paper Information
Paper Title:
Data--driven Image Restoration with Option--driven Learning for Big and Small Astronomical Image Datasets
Publication:
arXiv e-prints
Bibcode:
2020arXiv201103696J
Identifiers
DOI:
10.12149/101042
VO Identifier:
ivo://China-VO/paperdata/101042
Publication Date:
2020-11-10
Citation Guidelines
Jia, Peng et al. 2020. Data-driven image restoration with option-driven learning for big and small astronomical image data sets. Version 1.0. https://doi.org/10.12149/101042
@misc{10.12149/101042,
doi = {10.12149/101042},
url = {https://doi.org/10.12149/101042},
author = {Jia, Peng},
title = {Data-driven image restoration with option-driven learning for big and small astronomical image data sets},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2020}
}
Versions
Version 1.0 (current)
2020-11-10
Main
This DOI represents all versions, and will always resolve to the latest one.
2020-11-17