Kavli Affiliate: Lijing Shao | Summary:Discovery and timing observations of a radio pulsar orbiting around Sagittarius A*, the supermassive black hole (SMBH) in our Galactic Centre (GC), will provide unprecedented opportunities of studying the SMBH spacetime, testing gravity theories, and probing the astrophysical environment in the GC. However, unknown mass distributions might cause timing residuals […]
Continue.. Granular mass perturbations on the pulsar – supermassive black hole system