14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Pennsylvania State UniversityUS287 papers
- California Institute of TechnologyUS283 papers
- Goddard Space Flight CenterUS272 papers
- Massachusetts Institute of TechnologyUS255 papers
- Max Planck Institute for Gravitational PhysicsDE253 papers
- University of BirminghamGB250 papers
- University of GlasgowGB250 papers
- Hobart and William Smith CollegesUS244 papers
- University of Wisconsin–MilwaukeeUS244 papers
- Louisiana State UniversityUS241 papers
- University of FloridaUS240 papers
- Cardiff UniversityGB239 papers
11 papers · 2 filters
The effects of LIGO detector noise on a 15-dimensional Markov-chain Monte-Carlo analysis of gravitational-wave signals
V. Raymond, M. V. van der Sluys, I. Mandel +3
Gravitational-wave signals from inspirals of binary compact objects (black holes and neutron stars) are primary targets of the ongoing searches by ground-based gravitational-wave (…
Bayesian reconstruction of gravitational wave burst signals from simulations of rotating stellar core collapse and bounce
Christian Röver, Marie-Anne Bizouard, Nelson Christensen +3
Presented in this paper is a technique that we propose for extracting the physical parameters of a rotating stellar core collapse from the observation of the associated gravitation…
Status of NINJA: the Numerical INJection Analysis project
Benjamin Aylott, John G. Baker, William D. Boggs +74
The 2008 NRDA conference introduced the Numerical INJection Analysis project (NINJA), a new collaborative effort between the numerical relativity community and the data analysis co…
Einstein@Home search for periodic gravitational waves in early S5 LIGO data
LIGO Scientific Collaboration
This paper reports on an all-sky search for periodic gravitational waves from sources such as deformed isolated rapidly-spinning neutron stars. The analysis uses 840 hours of data…
Parameter estimation for signals from compact binary inspirals injected into LIGO data
Marc van der Sluys, Ilya Mandel, Vivien Raymond +3
During the fifth science run of the Laser Interferometer Gravitational-wave Observatory (LIGO), signals modelling the gravitational waves emitted by coalescing non-spinning compact…
Search for Gravitational Waves from Low Mass Compact Binary Coalescence in 186 Days of LIGO's fifth Science Run
The LIGO Scientific Collaboration
We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35 Msun, using LIGO observations between November 14, 2006 and May 18, 2…
Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data
The LIGO Scientific Collaboration, B. Abbott
According to general relativity a perturbed black hole will settle to a stationary configuration by the emission of gravitational radiation. Such a perturbation will occur, for exa…
Search for gravitational-wave bursts in the first year of the fifth LIGO science run
LIGO Scientific Collaboration, B. P. Abbott
We present the results obtained from an all-sky search for gravitational-wave (GW) bursts in the 64-2000 Hz frequency range in data collected by the LIGO detectors during the first…
Search for High Frequency Gravitational Wave Bursts in the First Calendar Year of LIGO's Fifth Science Run
LIGO Scientific Collaboration, B. Abbott
We present an all-sky search for gravitational waves in the frequency range 1 to 6 kHz during the first calendar year of LIGO's fifth science run. This is the first untriggered LIG…
Testing gravitational-wave searches with numerical relativity waveforms: Results from the first Numerical INJection Analysis (NINJA) project
Benjamin Aylott, John G. Baker, William D. Boggs +74
The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave data analysis communities. The purpose…
Search for Gravitational Waves from Low Mass Binary Coalescences in the First Year of LIGO's S5 Data
LIGO Scientific Collaboration, B. Abbott
We have searched for gravitational waves from coalescing low mass compact binary systems with a total mass between 2 and 35 Msun and a minimum component mass of 1 Msun using data f…