Maria Principe
Maria Principe
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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
12398*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
32102016
Multi-messenger observations of a binary neutron star merger
BP Abbott, S Bloemen, P Canizares, H Falcke, RP Fender, S Ghosh, ...
2370*2017
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
21832017
Advanced ligo
J Aasi, BP Abbott, R Abbott, T Abbott, MR Abernathy, K Ackley, C Adams, ...
Classical and quantum gravity 32 (7), 074001, 2015
20552015
GW170814: a three-detector observation of gravitational waves from a binary black hole coalescence
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
Physical review letters 119 (14), 141101, 2017
17072017
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
16712017
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
15072009
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
12972010
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
12762016
Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA
BP Abbott, R Abbott, TD Abbott, S Abraham, F Acernese, K Ackley, ...
Living reviews in relativity 23 (1), 1-69, 2020
11402020
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
9352017
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
8392018
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
8052011
A gravitational-wave standard siren measurement of the Hubble constant
LIGO Scientific Collaboration, Virgo Collaboration, 1M2H Collaboration, ...
Nature 551 (7678), 85-88, 2017
7262017
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
7142016
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
6242016
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
5982017
Properties of the binary neutron star merger GW170817
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley, C Adams, T Adams, ...
Physical Review X 9 (1), 011001, 2019
4982019
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
4862016
Il sistema al momento non pu eseguire l'operazione. Riprova pi tardi.
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