Radio astronomical images object detection and segmentation: a benchmark on deep learning methods

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Experimental Astronomy Pub Date : 2023-05-05 DOI:10.1007/s10686-023-09893-w
Renato Sortino, Daniel Magro, Giuseppe Fiameni, Eva Sciacca, Simone Riggi, Andrea DeMarco, Concetto Spampinato, Andrew M. Hopkins, Filomena Bufano, Francesco Schillirò, Cristobal Bordiu, Carmelo Pino
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引用次数: 2

Abstract

In recent years, deep learning has been successfully applied in various scientific domains. Following these promising results and performances, it has recently also started being evaluated in the domain of radio astronomy. In particular, since radio astronomy is entering the Big Data era, with the advent of the largest telescope in the world - the Square Kilometre Array (SKA), the task of automatic object detection and instance segmentation is crucial for source finding and analysis. In this work, we explore the performance of the most affirmed deep learning approaches, applied to astronomical images obtained by radio interferometric instrumentation, to solve the task of automatic source detection. This is carried out by applying models designed to accomplish two different kinds of tasks: object detection and semantic segmentation. The goal is to provide an overview of existing techniques, in terms of prediction performance and computational efficiency, to scientists in the astrophysics community who would like to employ machine learning in their research.

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射电天文图像目标检测和分割:深度学习方法的基准
近年来,深度学习已经成功地应用于各个科学领域。随着这些有希望的结果和表现,它最近也开始在射电天文学领域进行评估。特别是,随着射电天文学进入大数据时代,随着世界上最大的望远镜——平方公里阵列(SKA)的出现,自动目标检测和实例分割任务对于源的发现和分析至关重要。在这项工作中,我们探索了最被肯定的深度学习方法的性能,应用于无线电干涉仪器获得的天文图像,以解决自动源检测的任务。这是通过应用用于完成两种不同任务的模型来实现的:对象检测和语义分割。目标是提供现有技术的概述,在预测性能和计算效率方面,天体物理学界的科学家们希望在他们的研究中使用机器学习。
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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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