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.
翻译:近年来,在各种科学领域成功地应用了深层次的学习,在这些有希望的成果和表现之后,最近还开始在射电天文学领域对其进行评价,特别是由于射电天文学正在进入大数据时代,随着世界上最大的望远镜-Square Kilom Array(SKA)的出现,自动物体探测和实例分解的任务对于来源的发现和分析至关重要。在这项工作中,我们探索了最坚定的深层次学习方法的绩效,这些方法应用于通过无线电干涉测量仪器获得的天文图像,以解决自动源探测的任务。这是通过应用旨在完成两种不同任务的模型来完成的:物体探测和语义分解。目标是向天文学界的科学家提供预测性能和计算效率方面的现有技术概览,他们希望在研究中使用机器学习的方法。</s>