activity
20032025
most citedAnalysis of LIGO data for gravitational waves from binary neutron stars

196 citations · 1.1k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.IM2025

Impact of phase signal formulations on tilt-to-length coupling noise in the LISA test mass interferometer

Paul Edwards, Megha Dave, Alexander Weaver +4

Tilt-to-length (TTL) coupling in the Laser Interferometer Space Antenna (LISA) can generate spurious displacement noise that potentially affects the measurement of gravitational wa…

physics.optics2017★ 24 cited

Quantum correlation measurements in interferometric gravitational wave detectors

D. V. Martynov, V. V. Frolov, S. Kandhasamy +199

Quantum fluctuations in the phase and amplitude quadratures of light set limitations on the sensitivity of modern optical instruments. The sensitivity of the interferometric gravit…

physics.ins-det2016★ 4 cited

Small optic suspensions for Advanced LIGO input optics and other precision optical experiments

G. Ciani, M. A. Arain, S. M. Aston +13

We report on the design and performance of small optic suspensions developed to suppress seismic motion of out-of-cavity optics in the Input Optics subsystem of the Advanced LIGO i…

hep-ph2013★ 154 cited

Dark Sectors and New, Light, Weakly-Coupled Particles

R. Essig, J. A. Jaros, W. Wester +86

Dark sectors, consisting of new, light, weakly-coupled particles that do not interact with the known strong, weak, or electromagnetic forces, are a particularly compelling possibil…

astro-ph.HE2012★ 78 cited

Implications For The Origin Of GRB 051103 From LIGO Observations

The LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +568

We present the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically det…

astro-ph.CO2011★ 110 cited

Directional limits on persistent gravitational waves using LIGO S5 science data

J. Abadie, B. P. Abbott, R. Abbott +712

The gravitational-wave (GW) sky may include nearby pointlike sources as well as astrophysical and cosmological stochastic backgrounds. Since the relative strength and angular distr…