J Woehler
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Explore the profile of J Woehler including associated specialties, affiliations and a list of published articles.
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Articles
19
Citations
217
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Recent Articles
11.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Living Rev Relativ
. 2018 May;
21(1):3.
PMID: 29725242
We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to...
12.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2018 Mar;
120(9):091101.
PMID: 29547330
The LIGO Scientific and Virgo Collaborations have announced the event GW170817, the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron...
13.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2018 Feb;
120(3):031104.
PMID: 29400511
We present results from the first directed search for nontensorial gravitational waves. While general relativity allows for tensorial (plus and cross) modes only, a generic metric theory may, in principle,...
14.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2017 Nov;
119(16):161101.
PMID: 29099225
On August 17, 2017 at 12∶41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected...
15.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2017 Oct;
119(14):141101.
PMID: 29053306
On August 14, 2017 at 10∶30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar...
16.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2017 Jun;
118(22):221101.
PMID: 28621973
We describe the observation of GW170104, a gravitational-wave signal produced by the coalescence of a pair of stellar-mass black holes. The signal was measured on January 4, 2017 at 10∶11:58.6...
17.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2017 Apr;
118(12):121102.
PMID: 28388200
We employ gravitational-wave radiometry to map the stochastic gravitational wave background expected from a variety of contributing mechanisms and test the assumption of isotropy using data from the Advanced Laser...
18.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2017 Apr;
118(12):121101.
PMID: 28388180
A wide variety of astrophysical and cosmological sources are expected to contribute to a stochastic gravitational-wave background. Following the observations of GW150914 and GW151226, the rate and mass of coalescing...
19.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2016 Jul;
116(24):241103.
PMID: 27367379
We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer...