通过预训练进行有效的星系分类

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Jesse Schneider, D. Stenning, L. Elliott
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引用次数: 0

摘要

深度学习越来越多地应用于天文学中的监督学习任务,例如根据星系的表观形状对其图像进行分类(即星系形态分类),以深入了解星系的演化。在这项工作中,我们研究了预训练对经典AlexNet卷积神经网络(CNN)在对斯隆数字巡天数据发布4中的14034个星系的图像进行分类时的性能的影响。预训练涉及在与天文学无关的大型标记图像数据集上设计和训练细胞神经网络,与相对少量的标记星系图像相比,这利用了大量可用的此类数据。我们展示了使用预训练在统计上的显著优势,无论是在提高总体分类成功率方面,还是在降低计算成本以实现这种性能方面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Efficient galaxy classification through pretraining
Deep learning has increasingly been applied to supervised learning tasks in astronomy, such as classifying images of galaxies based on their apparent shape (i.e., galaxy morphology classification) to gain insight regarding the evolution of galaxies. In this work, we examine the effect of pretraining on the performance of the classical AlexNet convolutional neural network (CNN) in classifying images of 14,034 galaxies from the Sloan Digital Sky Survey Data Release 4. Pretraining involves designing and training CNNs on large labeled image datasets unrelated to astronomy, which takes advantage of the vast amounts of such data available compared to the relatively small amount of labeled galaxy images. We show a statistically significant benefit of using pretraining, both in terms of improved overall classification success and reduced computational cost to achieve such performance.
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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