Parkes observations for project P574 semester 2017APRS_BPSR_06

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 find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we\r\nare (co-)authors on 50 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from Bordeaux, Stanford, Swinburne and Oxford.

我们申请了观测时长以定期观测260颗脉冲星，旨在为利用费米卫星（Fermi Satellite）探测与表征伽马射线脉冲星提供所需的精确脉冲星计时星历表。
本项目的核心科学目标包括：扩充已知伽马射线脉冲星（涵盖射电明亮型与射电静默型）的数量；获取高精度脉冲轮廓；并表征其高能（相位分辨）能谱。
在射电波段开展的观测还将助力我们发现脉冲星突跳、表征计时噪声，研究色散与旋转测量变异性，并深化对单脉冲现象学的认知。
截至目前，我们作为（共同）作者已依托本合作与P574数据集发表了50篇学术论文。本数据集还支撑了来自波尔多大学、斯坦福大学、斯威本科技大学与牛津大学的学生完成其博士学位论文。