David Ottaway
Title
Cited by
Cited by
Year
Observation of gravitational waves from a binary black hole merger
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (6), 061102, 2016
10304*2016
GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (24), 241103, 2016
27872016
Advanced ligo
J Aasi, BP Abbott, R Abbott, T Abbott, MR Abernathy, K Ackley, C Adams, ...
Classical and quantum gravity 32 (7), 074001, 2015
2135*2015
GW170104: observation of a 50-solar-mass binary black hole coalescence at redshift 0.2
L Scientific, BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, ...
Physical Review Letters 118 (22), 221101, 2017
19502017
Multi-messenger observations of a binary neutron star merger
BP Abbott, S Bloemen, P Canizares, H Falcke, RP Fender, S Ghosh, ...
16762017
Gravitational waves and gamma-rays from a binary neutron star merger: GW170817 and GRB 170817A
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
The Astrophysical Journal Letters 848 (2), L13, 2017
14392017
Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors
J Abadie, BP Abbott, R Abbott, M Abernathy, T Accadia, F Acernese, ...
Classical and Quantum Gravity 27 (17), 173001, 2010
1428*2010
LIGO: the laser interferometer gravitational-wave observatory
BP Abbott, R Abbott, R Adhikari, P Ajith, B Allen, G Allen, RS Amin, ...
Reports on Progress in Physics 72 (7), 076901, 2009
14192009
Binary black hole mergers in the first advanced LIGO observing run
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical Review X 6 (4), 041015, 2016
11032016
GW170608: Observation of a 19 solar-mass binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
The Astrophysical Journal Letters 851 (2), L35, 2017
7982017
Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light
J Aasi, J Abadie, BP Abbott, R Abbott, TD Abbott, MR Abernathy, C Adams, ...
Nature Photonics 7 (8), 613-619, 2013
7002013
A gravitational wave observatory operating beyond the quantum shot-noise limit
J Abadie, BP Abbott, R Abbott, TD Abbott, M Abernathy, C Adams, ...
Nature Physics 7 (12), 962, 2011
6972011
GWTC-1: a gravitational-wave transient catalog of compact binary mergers observed by LIGO and Virgo during the first and second observing runs
BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, ...
Physical Review X 9 (3), 031040, 2019
6642019
Properties of the binary black hole merger GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (24), 241102, 2016
6322016
GW170817: Measurements of neutron star radii and equation of state
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
Physical review letters 121 (16), 161101, 2018
5762018
Exploring the sensitivity of next generation gravitational wave detectors
BP Abbott, R Abbott, TD Abbott, MR Abernathy, K Ackley, C Adams, ...
Classical and Quantum Gravity 34 (4), 044001, 2017
4452017
An upper limit on the stochastic gravitational-wave background of cosmological origin
LIGO Scientific Collaboration, Virgo Collaboration
arXiv preprint arXiv:0910.5772, 2009
4422009
An all-optical trap for a gram-scale mirror
T Corbitt, Y Chen, E Innerhofer, H Müller-Ebhardt, D Ottaway, H Rehbein, ...
Physical review letters 98 (15), 150802, 2007
4382007
GW150914: The Advanced LIGO detectors in the era of first discoveries
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (13), 131103, 2016
4142016
Detector description and performance for the first coincidence observations between LIGO and GEO
B Abbott, R Abbott, R Adhikari, A Ageev, B Allen, R Amin, SB Anderson, ...
Nuclear Instruments and Methods in Physics Research Section A: Accelerators …, 2004
3932004
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