LIGO Document G1901954-v3
- The low-mass X-ray binary Scorpius X-1 is a promising source of continuous gravitational waves. Its high X-ray luminosity indicates a large rate of accretion, which may power GW emission. A variety of methods have been developed and applied to search for a GW signal, which presents challenges because of the unknown signal frequency and residual uncertainties in orbital parameters. I will summarize the search results from Advanced LIGO and Advanced Virgo's first two Observing Runs (O1 and O2), and describe prospects for searches in the O3 run.
DCC Version 3.4.3, contact
Document Database Administrators