Parkes observations for project P574 semester 2023APRS_05

We request time to observe 260 pulsars on a regular basis in order to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to characterise their high energy (phase-resolved) spectra. In the radio, the observations will also allow us to investigate: neutron stars and pulsar emission via detecting glitches and determining pulse timing parameters; and the ISM via measuring and monitoring dispersion measures, Faraday rotation measures, and scintillation. To date, we are (co-)authors on over 95 papers arising from the collaboration and P574 data, including four which use UWL observations. The data have contributed to the PhD theses of students from Bordeaux, Manchester, Oxford, Stanford, and Swinburne.我们申请了望远镜观测时长，以定期开展260颗脉冲星的观测工作，旨在为利用费米卫星（Fermi satellite）探测与表征γ射线脉冲星提供必需的精确星历表（ephemerides）。本项目的核心科学目标包括：扩充已知γ射线脉冲星的样本量（涵盖射电亮与射电宁静两类），获取高精度脉冲轮廓，并表征其高能（相位分辨）能谱。在射电波段的观测还将支持多项研究：通过探测脉冲星自转突变（glitch）并测定脉冲计时参数，开展中子星与脉冲星辐射机制研究；通过测量与监测色散量、法拉第旋转量以及射电闪烁，研究星际介质（Interstellar Medium，ISM）。截至目前，基于本合作项目与P574数据集产出的学术成果，我们作为共同作者已参与发表超过95篇论文，其中4篇利用了UWL观测数据。相关数据集还助力了来自波尔多大学、曼彻斯特大学、牛津大学、斯坦福大学以及斯威本科技大学的学生完成其博士学位论文。