Statistical cosmology from standard siren gravitational wave events

有了计划中的未来引力波观测站，如LISA，再加上欧几里得等强大的望远镜，我们探索这两个窗口如何相互补充，了解宇宙的内容和动力学是至关重要的。利用紧致双星合并的光度距离和星系巡天的红移发现的引力波弱透镜效应就是这种互补信息的一个例子——在这个项目中，它的潜力将被详细探索。

With planned future gravitational wave observatories such as LISA, coupled with powerful telescopes such as Euclid, it is vital we explore how these two windows into the content and dynamics of the Universe can complement one another. The weak lensing of gravitational waves found using luminosity distances obtained from compact binary coalescences and redshifts from galaxy surveys is an example of such complementary information - in this project its potential will be explored in detail.