402 citations · 2k across the 58 of their papers we have counts for
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Prospects for LISA to detect a gravitational-wave background from first order phase transitions
Guillaume Boileau, Nelson Christensen, Chloe Gowling +2
First order phase transitions in the early universe could produce a gravitational-wave background that might be detectable by the Laser Interferometer Space Antenna (LISA). Such an…
Impact of correlated seismic and correlated Newtonian noise on the Einstein Telescope
Kamiel Janssens, Guillaume Boileau, Nelson Christensen +2
Correlated noise could impact the search for the gravitational wave background at future Earth-based gravitational-wave detectors. Due to the small distance ( 400 m) between…
Formalism for power spectral density estimation for non-identical and correlated noise using the null channel in Einstein Telescope
Kamiel Janssens, Guillaume Boileau, Marie-Anne Bizouard +3
Several proposed gravitational wave interferometers have a triangular configuration, such as the Einstein Telescope and the Laser Interferometer Space Antenna. For such a configura…
Cosmology with the Laser Interferometer Space Antenna
Pierre Auclair, David Bacon, Tessa Baker +177
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravita…
Figures of merit for a stochastic gravitational-wave background measurement by LISA: implications of LISA Pathfinder noise correlations
Guillaume Boileau, Nelson Christensen, Renate Meyer
An important goal of the Laser Interferometer Space Antenna (LISA) is to observe a stochastic gravitational-wave background (SGWB). A study of possible correlated noise in LISA is…