Parkes observations for project P1092 semester 2020OCTS_04

We propose to use the Parkes UWL receiver for confirmation and monitoring a sub-set of bright FAST-discovered pulsars, especially for those discoveries located outside the sky regions covered by the purchased PX-500 project. For special FAST discoveries that already confirmed by Parkes, such as MSPs or pulsars with interesting emission properties, we propose to do long-term monitoring for them as well. These monitoring aim to solve their parameters, binary orbit, and provide significant insight into the special emission properties of these new discoveries and facilitate science. The Parkes UWL system provides a unique capability for studying the pulsars over wide bandwidths, in term of both the timing precision and frequency-dependent observing properties.

我们提议使用帕克斯（Parkes）UWL接收机，对由500米口径球面射电望远镜（Five-hundred-meter Aperture Spherical radio Telescope，FAST）发现的一批亮脉冲星开展证认与监测工作，重点针对那些位于已购置的PX-500项目覆盖天区之外的FAST发现脉冲星。对于已由帕克斯望远镜证认的特殊FAST发现脉冲星，例如毫秒脉冲星（Millisecond Pulsars, MSPs）或具备特殊辐射特性的脉冲星，我们同样提议对其开展长期监测。此类监测旨在精确测定这些脉冲星的物理参数与双星轨道参数，为深入理解这批新发现脉冲星的特殊辐射特性提供重要洞见，并助力相关科学研究推进。帕克斯UWL系统在宽频段脉冲星研究中具备独特优势，在计时精度与频率相关观测特性两方面均表现出色。