Parkes observations for project P1032 semester 2023APRS_01

This project aims to continue to perform rapid measurements of relativistic parameters of southern binary pulsar systems using data from the Parkes Ultra Wideband Low (UWL) receiver and the MeerKAT telescope thereby enabling measurement of their component masses and in some cases, test theories of gravity. We will use the UWL data to obtain significant orbital coverage and timing baseline on these pulsars and obtain important constraints on orbital and temporal DM variations that will help in identifying the nature of the companion star. We will then use MeerKAT data at crucial orbital phases to improve our chances of measuring the relativistic parameters. Increase in the number of measured NS masses has profound implications for NS internal structure and for stellar and binary evolution physics.

本项目旨在依托帕克斯（Parkes）超宽带低（Ultra Wideband Low, UWL）接收机与梅尔克特（MeerKAT）望远镜的观测数据，持续开展南天双星脉冲星系统的相对论参数快速测量工作，以此实现对其组分质量的测定，并在部分研究案例中验证引力理论。本研究将利用UWL观测数据，获取这些脉冲星的有效轨道覆盖范围与计时基线，并对轨道与时域色散量（Dispersion Measure, DM）变化给出重要约束条件，从而助力明确其伴星的物理性质。后续我们将利用关键轨道相位下的梅尔克特望远镜观测数据，提升相对论参数的测量成功率。已测得的中子星（Neutron Star, NS）质量样本数量的增加，对于中子星内部结构研究以及恒星与双星演化物理学领域均具有深远意义。