Parameter Estimation

We have applied the deep learning model, GW-SkyLocator, to demonstrate for the first time, that gravitational wave signals from binray neutron star mergers can be localized before merger.

We have developed a deep learning model, called GW-SkyLocator, to obtain the posterior distribution of the sky location of gravitational wave sources. This method is applicable for all three categories of compact binary coalescences - binary black holes, binary neutron stars and neutron star-black hole binaries.