📝 SummarXiv

Abstract

During LIGO s third observing run (O3), simulated continuous gravitational wave (CW) signals were added to the detectors via hardware (HW) injections, which are physical injections into the interferometer control loop. These included two periodic signals mimicking a spinning neutron star in a binary system, similar to the low-mass X-ray binary Scorpius X-1 (Sco X-1). HW injections serve as an important validation of a search method, as they occur before data cleaning and preparation. We searched for these injections using a cross-correlation pipeline, which searched for CWs from Sco X-1 in the O3 run. To simulate a realistic search, we used a search region of orbital parameter space of similar size to the plausible parameter ranges for Sco X-1, but containing the parameters of each HW injection. Our self-blinded analysis confidently detects one of the injections. The other, which was generated with a lower amplitude and in a more expensive region of frequency space, was not detected. We verified the imprint of this second signal by performing a deeper targeted search at its true parameters. However, such a deep search across the full parameter range would have been computationally infeasible.