Focal-Field Reconstruction for Astronomical Transients with Conditional Generative Adversarial Networks

Decheng Wu, Nanjie Lv, H. Cao, Jin Fan, Lisheng Yang, Shi-zhong Yang
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Abstract

Since fast transients such as fast radio bursts (FRBs) are short-duration events, the telescope should require a wide instantaneous field of view $(\mathbf{FoV})$. Unlike traditional beam-scanning technology, this paper $\mathbf{p}$ roposes a new approach for transient radio target detection using focal-field feature matching. As for traditional phased array feed (PAF) telescope with few array elements, the features of focal-field distribution (FFD) are very limited. Exploiting the strong fitting ability of the neural networks, a generative adversarial networks (GANs)-based method is presented to reconstruct FFD features. Moreover, according to the abundant frequency characteristic of the FRBs, a multiple-frequency joint estimation is used to constrain the reconstruction. A shrunken Five-hundred-meter Aperture Spherical radio Telescope (FAST) model is utilized to verify the effectiveness of the method. The simulation results demonstrate that this approach can reconstruct the FFD effectively only using limited feeds and relative accurately estimate the transient position.
基于条件生成对抗网络的天文瞬态焦场重建
由于像快速射电暴(frb)这样的快速瞬变是持续时间很短的事件,望远镜应该需要一个宽的瞬时视场$(\mathbf{FoV})$。与传统的波束扫描技术不同,本文提出了一种基于焦场特征匹配的瞬态无线电目标检测新方法。传统的相控阵馈源(PAF)望远镜阵元较少,其焦场分布特性非常有限。利用神经网络强大的拟合能力,提出了一种基于生成对抗网络(GANs)的FFD特征重构方法。此外,根据快速射电暴丰富的频率特性,采用多频联合估计约束重构。利用缩小500米口径球面射电望远镜(FAST)模型验证了该方法的有效性。仿真结果表明,该方法可以在有限馈入条件下有效地重构FFD,并相对准确地估计出瞬态位置。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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