Parkes observations for project P456 semester 2021OCTS_05

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. We are now in an exciting regime where a signal detected in our (and other data sets) has the form expected for a gravitational wave background. We are therefore now attempting to confirm, or deny, this exciting result. 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）项目共有三项核心目标：(a) 探测来自天文源的引力波；(b) 建立脉冲星时标系统；(c) 深化对太阳系动力学的认知。当前我们正处于一个令人振奋的研究阶段：我们的数据集（以及其他相关数据集）中探测到的信号，其形态符合引力波背景的预期特征。因此我们正尝试证实或证伪这一振奋人心的结果。通过本观测申请，我们旨在维持本领域的领先地位。

与多数观测申请不同，本申请属于持续性观测项目：相关观测将持续收紧超低频引力波的约束范围，直至最终探测到该信号。帕克斯望远镜的持续观测至少将保持其科研价值，直至平方公里阵列（Square Kilometre Array，SKA）第一阶段项目能够提升我们的观测灵敏度与观测节奏。即便引力波背景被成功探测，我们仍将持续开展观测，以支撑引力波天文学这一新兴领域的发展！