主讲人单位 (Speaker's Institute): 华南师范大学

邀请人 (Invited by): 张建东

时间 (Time): 星期三，2023/03/29-14:30-16:00

地点 (Location): 珠海校区天琴中心1416会议室

摘要 (Abstract): 

Astronomers interested in GWs who are not experts in this field sometimes need to get a quick idea of what GW sources can be detected by certain detectors, and the accuracy of the measured parameters. The GW-Toolbox is a set of easy-to-use, flexible tools to simulate observations of the GW universe with different detectors. We include a broad range of sources, such as mergers of stellar-mass compact objects, namely black holes, neutron stars, and black hole-neutron star binaries, supermassive black hole binary mergers and inspirals, Galactic double white dwarfs in ultra-compact orbit, extreme-mass-ratio inspirals, and stochastic GW backgrounds. 

In this talk, I will give a throughout overview of the toolbox, including its functionalities and methodology. I will also present two recent scientific application works done with the toolbox, namely the study on the future prospect of GW astronomy on binary black hole population and sub-threshold joint observation on binary neutron star mergers as GW sources and gamma-ray bursts.
 

主讲人简介 (Speaker's CV): 

易疏序，2010年毕业于清华大学物理系；2016年自中国科学大学获得天体物理博士学位；2016年至2021年先后在香港大学、荷兰拉德堡德大学从事博士后研究；2022作为青年特聘研究员就职于中科院高能物理研究所。研究领域包括：致密天体的引力波及高能辐射，天文软件开发等。