Parkes observations for project PX600 semester 2020APRS_07

The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the GC is widely cited as a location believed to harbour advanced civilizations, and it is also the most energetic region in the Milky Way. We aim to conduct BL-GC Survey with Parkes radio telescope for around 350 hours. We will cover the frequency range from 700 MHz to 4 GHz, utilizing the newly installed ultra-wideband receiver. Our team has already leveraged both standard and bespoke tools to construct a flexible software stack to search data for signals of interest. We will look for signals from extraterrestrial intelligence (ETI) by searching for both simple narrow-band signals and complex modulated signals. Along with that, as an ancillary science, we will also search for accelerated pulsars — likely orbiting a supermassive black hole at the centre of the Milky Way Galaxy. Data products produced during this program will also be publically available to engage larger pulsar community

银心（Galactic Center, GC）是突破聆听（Breakthrough Listen, BL）项目射电波段的核心观测目标。作为天空中任一方向恒星数量最多的天区，银心常被视作存在先进文明的候选区域，同时也是银河系内能量最为活跃的区域。本项目计划使用帕克斯射电望远镜开展BL-GC巡天观测，总时长约350小时，观测将覆盖700 MHz至4 GHz的频段，并采用新安装的超宽带接收机。本团队已整合标准工具与定制化工具，搭建了一套灵活的软件栈，用于从观测数据中搜寻目标信号。我们将通过搜寻简易窄带信号与复杂调制信号两种类型，来寻找地外智慧文明（extraterrestrial intelligence, ETI）发出的信号。与此同时，作为辅助科学研究内容，我们还将搜寻加速脉冲星——这类天体大概率绕银河系中心的超大质量黑洞运行。本项目产生的所有数据产品都将对外公开，以服务于更广泛的脉冲星研究群体。