649 citations · 3.1k across the 35 of their papers we have counts for
35 papers
Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
Sushant Sharma Chaudhary, Andrew Toivonen, Gaurav Waratkar +50
Multi-messenger searches for BNS and NSBH mergers are currently one of the most exciting areas of astronomy. The search for joint electromagnetic and neutrino counterparts to GWs h…
Adapting the PyCBC pipeline to find and infer the properties of gravitational waves from massive black hole binaries in LISA
Connor R. Weaving, Laura K. Nuttall, Ian W. Harry +2
The Laser Interferometer Space Antenna (LISA), due for launch in the mid 2030s, is expected to observe gravitational waves (GW)s from merging massive black hole binaries (MBHB)s. T…
Space-based Gravitational Wave Observatories Will Be Able to Use Eccentricity to Unveil Stellar-mass Binary Black Hole Formation
Han Wang, Ian Harry, Alexander Nitz +1
The measurement of eccentricity would provide strong constraints on the formation channel of stellar-mass binary black holes. However, current ground-based gravitational wave detec…
A search technique to observe precessing compact binary mergers in the advanced detector era
Connor McIsaac, Charlie Hoy, Ian Harry
Gravitational-wave signals from compact binary coalescences are most efficiently identified through matched filter searches, which match the data against a pre-generated bank of gr…
ArchEnemy: Removing scattered-light glitches from gravitational wave data
Arthur E. Tolley, Gareth S. Cabourn Davies, Ian W. Harry +1
Data recorded by gravitational wave detectors includes many non-astrophysical transient noise bursts, the most common of which is caused by scattered-light within the detectors. Th…
Addressing the challenges of detecting time-overlapping compact binary coalescences
Philip Relton, Andrea Virtuoso, Sophie Bini +6
Standard detection and analysis techniques for transient gravitational waves make the assumption that detector data contains, at most, one signal at any time. As detectors improve…