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Parkes observations for project P456 semester 2008OCTS

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Research Data Australia2024-12-14 收录
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https://researchdata.edu.au/parkes-observations-project-semester-2008octs/445359
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The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. There are many secondary goals, some astrophysical and some instrumental/technique oriented. Achievement of these ambitious primary goals requires frequent observations of at least 20 MSPs at two or preferably three widely spaced frequencies over several years. We wish to continue observing the PPTA sample at intervals of 2-3 weeks using both the 10/50cm and Multibeam receivers. The digital filterbanks (PDFB2, PDFB3) and the baseband systems (CPSR2; APSR soon) are used for data recording. With the new instruments and development of an efficient pipeline processing system, we are getting the world's best pulsar timing precision, with four pulsars having rms residuals of less than 200 ns and more than half less than 1 microsecond. We are collaborating with the European and North American pulsar timing array groups (EPTA and NANOGrav, respectively) to obtain more frequent observations and a larger pulsar sample. Because of the high sensitivity and wide bandwidths required, RFI mitigation is an important part of the project.

帕克斯脉冲星计时阵列(Parkes Pulsar Timing Array, PPTA)项目设有三大核心目标:(a) 探测来自各类天文源的引力波;(b) 建立标准化脉冲星时标;(c) 深化对太阳系动力学机制的认知。该项目同时兼具诸多次级目标,涵盖天体物理与仪器/技术两大研究方向。要达成这些极具雄心的核心目标,需在数年周期内,以高频观测至少20颗毫秒脉冲星(Millisecond Pulsar, MSP),并在两个乃至三个间距较大的频率波段上开展观测。我们计划以2至3周的间隔持续观测PPTA样本,同步采用10/50厘米口径接收机与多波束接收机。数据记录环节采用数字滤波器组(PDFB2、PDFB3)与基带系统(CPSR2;APSR即将投入使用)。依托新型仪器设备与高效流水线处理系统的研发进展,我们已实现全球顶尖的脉冲星计时精度:目前已有4颗脉冲星的残差均方根值低于200纳秒,半数以上样本的残差均方根值小于1微秒。我们正与欧洲、北美脉冲星计时阵列团队(分别为EPTA与NANOGrav)开展合作,以获取更频繁的观测机会与更大规模的脉冲星样本。鉴于项目对高灵敏度与宽带宽的严苛需求,射频干扰(Radio Frequency Interference, RFI)抑制是该项目的重要组成环节。
搜集汇总
数据集介绍
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背景与挑战
背景概述
该数据集是Parkes脉冲星计时阵列(PPTA)项目在2008年10月至2009年3月期间的观测数据,旨在探测引力波、建立脉冲星时间尺度和研究太阳系动力学。它涉及对至少20颗毫秒脉冲星的高频观测,使用先进仪器实现纳秒级计时精度,并与国际团队合作以扩大样本。数据以开放许可发布,适用于天体物理研究。
以上内容由遇见数据集搜集并总结生成
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