Parkes observations for project P1338 semester 2024OCTS_42

Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a broad dichotomy in population has emerged. Some FRBs have been seen to be repeating, while others are not, despite a significant amount of follow-up using different radio telescopes. The repeating FRB 20240114A was recently discovered by CHIME/FRB, which has been seen to have an exceptionally high burst activity. Such extreme burst activity has not been seen in any other source. The repeating FRBs, such as FRB 20240114A, provide an unparalleled window into their circumburst environment due to their repeating nature, which can be used to constrain possible progenitor models and test underlying emission mechanisms. The previous Parkes/Murriyang source follow-up has also revealed intriguing spectro-polarimetric properties, such as frequency-dependent evolution of burst central frequency or chromaticity, a possible activity window, significantly large circular polarisation (CP), and frequency-dependent CP. These properties hold the key towards understanding the circumburst environment of the FRBs, and test possible progenitor models. A large bandwidth instrument with reliable polarimetry has been critical in uncovering these properties. The ultra-wideband low (UWL) receiver on Parkes/Murriyang is ideally suited to explore the source's wideband spectro-temporal and polarimetric behaviour. We propose a campaign to regularly follow up FRB 20240114A to ascertain its long-term evolution of spectro-temporal properties.

快速射电暴（Fast radio bursts, FRBs）是起源于河外的毫秒级射电暴。自从帕克斯/穆里扬存档的多波束观测数据中发现首例快速射电暴以来，该类天体的群体便呈现出鲜明的二分特性：尽管学界已借助多台射电望远镜开展了大量后续观测，但部分快速射电暴被证实会重复爆发，其余则仅出现单次爆发。CHIME/FRB合作组近期发现了重复快速射电暴20240114A，该暴展现出异常高的爆发活跃度，这类极端的爆发活跃度此前从未在其他天体中被观测到。诸如20240114A这类重复快速射电暴，凭借其重复爆发的特性，为研究其暴周环境提供了无与伦比的观测窗口，可用于约束潜在的前身天体模型并检验核心辐射机制。此前针对帕克斯/穆里扬望远镜发现的快速射电暴源开展的后续研究，还揭示了诸多引人关注的光谱偏振特性：例如暴中心频率的频率依赖演化（或称色特性）、可能存在的爆发活跃窗口、显著的圆偏振（CP）信号，以及圆偏振随频率变化的现象。这些特性是破解快速射电暴暴周环境、验证各类潜在前身天体模型的关键所在。具备可靠偏振测量能力的大带宽观测设备，是揭示这些特性的核心条件。帕克斯/穆里扬望远镜搭载的超宽带低频（UWL）接收机，恰好能够完美适配该源的宽带光谱时域与偏振特性研究。我们提议开展系统性观测计划，对快速射电暴20240114A进行常态化后续观测，以明确其光谱时域特性的长期演化规律。