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Dr Thomas S Adams
Dr Thomas S Adams
LAPP
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Title
Cited by
Cited by
Year
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
16004*2016
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
154752016
Advanced ligo
J Aasi, BP Abbott, R Abbott, T Abbott, MR Abernathy, K Ackley, C Adams, ...
Classical and quantum gravity 32 (7), 074001, 2015
41652015
Tests of general relativity with GW150914
BP Abbott, R Abbott, MR Abernathy, RX Adhikari, SB Anderson, K Arai, ...
Physical Review Letters 116 (22), Art. No. 221101, 2016
1950*2016
Binary black hole mergers in the first advanced LIGO observing run
LIGO Scientific Collaboration, Virgo Collaboration
arXiv preprint arXiv:1606.04856, 2016
1894*2016
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
13712013
Properties of the binary black hole merger GW150914
BP Abbott, G Cagnoli, J Degallaix, V Dolique, R Flaminio, M Granata, ...
10522016
Properties of the binary black hole merger GW150914
LIGO Scientific Collaboration, Virgo Collaboration
arXiv preprint arXiv:1602.03840, 2016
1052*2016
Astrophysical Implications of the Binary Black Hole Merger GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
The Astrophysical Journal Letters 818 (2), L22, 2016
8262016
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
7592016
Characterization of the LIGO detectors during their sixth science run
J Aasi, J Abadie, BP Abbott, R Abbott, T Abbott, MR Abernathy, T Accadia, ...
Classical and Quantum Gravity 32 (11), 115012, 2015
5812015
GW150914: First results from the search for binary black hole coalescence with Advanced LIGO
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical Review D 93 (12), 122003, 2016
5272016
Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Classical and Quantum Gravity 33 (13), 134001, 2016
4352016
Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
LIGO Scientific Collaboration, Virgo Collaboration
arXiv preprint arXiv:1602.03844, 2016
435*2016
GW150914: Implications for the stochastic gravitational-wave background from binary black holes
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (13), 131102, 2016
4332016
Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
arXiv preprint arXiv:1606.03939, 2016
375*2016
The rate of binary black hole mergers inferred from Advanced LIGO observations surrounding GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
arXiv preprint arXiv:1602.03842, 2016
3722016
Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network
J Aasi, J Abadie, BP Abbott, R Abbott, TD Abbott, M Abernathy, T Accadia, ...
Physical Review D 88 (6), 062001, 2013
336*2013
Localization and broadband follow-up of the gravitational-wave transient GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
arXiv preprint arXiv:1602.08492, 2016
301*2016
Search for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo data from 2009–2010
J Aasi, J Abadie, BP Abbott, R Abbott, TD Abbott, M Abernathy, T Accadia, ...
Physical Review D 87 (2), 022002, 2013
288*2013
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