activity
20142023
most citedGravitational-wave sensitivity curves

748 citations · 3.7k across the 47 of their papers we have counts for

collaborators

48 papers

physics.geo-ph2023

Modeling tsunammi inundation for hazard assessment of the Coral Coast of Fiji: Communities of Sigatoka and Cuvu

Diego Arcas, Christopher Moore

A tsunami hazard assessment was conducted for the communities of Sigatoka and Cuvu, located on the island of Viti Levu, Fiji. The study presents an overview of historical seismic a…

gr-qc2023★ 22 cited

LISA stellar-mass black hole searches with semicoherent and particle-swarm methods

Diganta Bandopadhyay, Christopher J. Moore

This paper considers the problem of searching for quiet, long-duration and broadband gravitational wave signals, such as stellar-mass binary black hole binaries, in mock LISA data.…

astro-ph.HE2023★ 4 cited

Implications of pulsar timing array observations for LISA detections of massive black hole binaries

Nathan Steinle, Hannah Middleton, Christopher J. Moore +6

Pulsar timing arrays (PTAs) and the Laser Interferometer Space Antenna (LISA) will open complementary observational windows on massive black-hole binaries (MBHBs), i.e., with masse…

gr-qc2023★ 4 cited

Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity

Roxana Rosca-Mead, Michalis Agathos, Christopher J. Moore +1

In massive scalar-tensor gravity, core-collapse supernovae are strong sources of scalar-polarized gravitational waves. These can be detectable out to large distance. The dispersive…

gr-qc2022★ 20 cited

On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences

Geraint Pratten, Antoine Klein, Christopher J. Moore +4

The observation of massive black hole binary systems is one of the main science objectives of the Laser Interferometer Space Antenna (LISA). The instrument's design requirements ha…

astro-ph.SR2022★ 47 cited

Identifying LISA verification binaries among the Galactic population of double white dwarfs

Eliot Finch, Giorgia Bartolucci, Daniel Chucherko +7

Double white dwarfs (DWDs) will be the most numerous gravitational-wave (GW) sources for the Laser Interferometer Space Antenna (LISA). Most of the Galactic DWDs will be unresolved…