Segui
Matthew R Abernathy
Matthew R Abernathy
Johns Hopkins University Applied Physics Lab
Email verificata su jhuapl.edu
Titolo
Citata da
Citata da
Anno
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
23363*2016
Advanced ligo
J Aasi, BP Abbott, R Abbott, T Abbott, MR Abernathy, K Ackley, C Adams, ...
Classical and quantum gravity 32 (7), 074001, 2015
6247*2015
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
30422016
The Einstein Telescope: A third-generation gravitational wave observatory
M Punturo, M Abernathy, F Acernese, B Allen, N Andersson, K Arun, ...
Classical and Quantum Gravity 27 (19), 194002, 2010
25702010
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
19212016
Tests of general relativity with GW150914
BP Abbott, R Abbott, TD Abbott, MR Abernathy, F Acernese, K Ackley, ...
Physical review letters 116 (22), 221101, 2016
18882016
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
14912013
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
13962010
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
13832017
A gravitational wave observatory operating beyond the quantum shot-noise limit
Nature Physics 7 (12), 962-965, 2011
11582011
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
11482016
Sensitivity studies for third-generation gravitational wave observatories
S Hild, M Abernathy, F Acernese, P Amaro-Seoane, N Andersson, K Arun, ...
Classical and Quantum gravity 28 (9), 094013, 2011
11212011
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
8712016
Scientific objectives of Einstein telescope
B Sathyaprakash, M Abernathy, F Acernese, P Ajith, B Allen, ...
Classical and Quantum Gravity 29 (12), 124013, 2012
7072012
Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy
DV Martynov, ED Hall, BP Abbott, R Abbott, TD Abbott, C Adams, ...
Physical Review D 93 (11), 112004, 2016
6482016
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
6132016
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
6022015
The third generation of gravitational wave observatories and their science reach
M Punturo, M Abernathy, F Acernese, B Allen, N Andersson, K Arun, ...
Classical and Quantum Gravity 27 (8), 084007, 2010
5252010
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
4632016
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
4552016
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