45 citations · 98 across the 11 of their papers we have counts for
6 papers · 1 filter
Premerger observation and characterization of massive black hole binaries
Gareth Cabourn Davies, Ian Harry, Michael J. Williams +11
We demonstrate an end-to-end technique for observing and characterizing massive black hole binary signals before they merge with the LISA space-based gravitational-wave observatory…
Cyclostationary signals in LISA: a practical application to Milky Way satellites
Federico Pozzoli, Riccardo Buscicchio, Antoine Klein +3
One of the primary sources of gravitational waves (GWs) anticipated to be detected by the Laser Interferometer Space Antenna (LISA) are Galactic double white dwarf binaries (DWDs).…
Test for LISA foreground Gaussianity and stationarity: galactic white-dwarf binaries
Riccardo Buscicchio, Antoine Klein, Valeriya Korol +4
Upcoming space-based gravitational-wave detectors will be sensitive to millions and resolve tens of thousands of stellar-mass binary systems at mHz frequencies. The vast majority o…
Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA
Alice Spadaro, Riccardo Buscicchio, David Izquierdo-Villalba +3
Massive black-hole binaries will be the loudest sources detectable by LISA. These systems are predicted to form during the hierarchical assembly of cosmic structures and coalesce b…
LISA Definition Study Report
Monica Colpi, Karsten Danzmann, Martin Hewitson +108
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves…
Efficient gravitational-wave model for fully-precessing and moderately-eccentric, compact binary inspirals
J. Nijaid Arredondo, Antoine Klein, Nicolás Yunes
Future gravitational-wave detectors, especially the Laser Interferometer Space Antenna (LISA), will be sensitive to black hole binaries formed in astrophysical environments that pr…