activity
20122026
most citedCharacterization of the LIGO detectors during their sixth science run

1.3k citations · 9.5k across the 88 of their papers we have counts for

collaborators
Showing 2016Show all

15 papers · 1 filter

gr-qc2016★ 42 cited

The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity

David Keitel, Xisco Jiménez Forteza, Sascha Husa +9

For a brief moment, a binary black hole (BBH) merger can be the most powerful astrophysical event in the visible universe. Here we present a model fit for this gravitational-wave p…

gr-qc2016★ 312 cited

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +992

A wide variety of astrophysical and cosmological sources are expected to contribute to a stochastic gravitational-wave background. Following the observations of GW150914 and GW1512…

gr-qc2016★ 102 cited

All-sky search for short gravitational-wave bursts in the first Advanced LIGO run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +986

We present the results from an all-sky search for short-duration gravitational waves in the data of the first run of the Advanced LIGO detectors between September 2015 and January…

astro-ph.HE2016★ 76 cited

Search for Gravitational Waves Associated with Gamma-Ray Bursts During the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B

LIGO Scientific Collaboration, Virgo Collaboration, IPN Collaboration +1002

We present the results of the search for gravitational waves (GWs) associated with -ray bursts detected during the first observing run of the Advanced Laser Interferometer Gravi…

gr-qc2016★ 138 cited

Effects of waveform model systematics on the interpretation of GW150914

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +999

Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models diffe…

gr-qc2016★ 202 cited

Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy

Xisco Jiménez-Forteza, David Keitel, Sascha Husa +3

Numerical relativity is an essential tool in studying the coalescence of binary black holes (BBHs). It is still computationally prohibitive to cover the BBH parameter space exhaust…