Parkes observations for project P456 semester 2018OCTS_28

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. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days at three different wavelengths. With this proposal we aim to maintain our pre-eminent position in the field.\r\n\r\nUnlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!

帕克斯脉冲星计时阵列（Parkes Pulsar Timing Array, PPTA）项目拥有三大核心目标：（a）探测来自天文天体的引力波；（b）建立脉冲星时标系统；（c）深化对太阳系动力学的认知。帕克斯脉冲星计时阵列是三个国际脉冲星计时研究团队中历史最悠久的一个。我们拥有规模最小的望远镜与研究团队，但却取得了最精良的测量数据与最出色的研究成果。我们针对非相干引力波背景强度给出的观测约束，是目前唯一能够有效限制相关理论模型的约束条件。我们始终保持领先地位的原因在于：我们拥有南天区观测视野；我们的团队规模小巧但目标聚焦；我们配备了校准精度最高的接收机；并且我们能够以15至20天的近乎恒定的观测周期，在三个不同射电波段开展观测。通过本提案，我们旨在巩固自身在该领域的领先地位。

与绝大多数观测提案不同，本提案属于持续性观测项目，其观测工作将持续优化超低频引力波的约束精度，直至最终实现直接探测。至少在平方千米阵（Square Kilometre Array, SKA）第一阶段项目能够提升其观测灵敏度与观测周期之前，帕克斯望远镜的持续观测仍将具备重要科研价值。即便引力波背景被成功探测之后，我们仍将继续开展观测，以支撑新兴的引力波天文学领域发展。