Parkes observations for project P892 semester 2016OCTS_BPSR_51

SUPERBx is an extension to the SUPERB survey which looks at the highest Galactic latitudes in a search for fast radio bursts (FRBs). Our most recent results show that there is a strong Galactic latitude dependence to FRB detectability with the detection rate being 4 times higher ~45 degrees and higher above the plane; this is where SUPERBx will focus its efforts from now on. SUPERBx uses optimised GPU codes to search for pulsars and fast radio bursts (FRBs), making discoveries in real time. Handling our data as it comes in is essential for the SKA Phase I era so this work applies directly to the high-data rates of next generation telescopes. The FRBs discovered (we have already discovered four FRBs in this project) will have much more associated information than all previous detections. Firstly our discovery lag is ~1 second, rather than months/years. The Parkes observations will be shadowed by other radio telescopes (in particular the refurbished Molonglo which has now reached a level of performance where it has independently discovered 3 FRBs in 2016) to allow localisation of the discovered FRBs, and a host of optical and high-energy telescopes will then be triggered as appropriate. This is key for identifying FRB host galaxies, so as to solve the mystery of their progenitors and to exploit their many uses as tools for precision cosmology measurements.

SUPERBx是SUPERB巡天的扩展项目，旨在观测银道面高纬度区域以搜寻快速射电暴（fast radio burst, FRB）。我们的最新研究结果显示，FRB的可探测性存在显著的银道纬度依赖性：在银道面上方约45度及更高纬度区域，探测率可达原先的4倍，这也将成为SUPERBx后续的核心观测重点。SUPERBx采用优化后的图形处理器（Graphics Processing Unit, GPU）代码开展脉冲星与快速射电暴（FRB）的搜寻工作，可实现实时天文发现。在平方千米阵列（Square Kilometre Array, SKA）第一阶段的观测背景下，实时处理流式传入的数据至关重要，因此本项目的技术方案可直接适配下一代望远镜的高数据率场景。本项目已发现的FRB（本项目目前已发现4例FRB）将拥有远超此前所有探测结果的关联信息。首先，本项目的发现延迟仅约1秒，而非数月乃至数年。帕克斯（Parkes）望远镜的观测将与其他射电望远镜协同开展——其中经过翻新的莫隆格洛（Molonglo）望远镜目前已达到可独立完成探测的性能水准，并于2016年独立发现3例FRB——以此实现对已发现FRB的精确定位；随后将根据观测需求触发多台光学与高能望远镜开展后续观测。这对于确定FRB的宿主星系、破解其起源之谜，以及将其作为精密宇宙学测量工具加以利用均具有关键意义。