C C Yancey
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Explore the profile of C C Yancey including associated specialties, affiliations and a list of published articles.
Author names and details appear as published. Due to indexing inconsistencies, multiple individuals may share a name, and a single author may have variations. MedLuna displays this data as publicly available, without modification or verification
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Articles
29
Citations
514
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Recent Articles
21.
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...
22.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2016 Jul;
116(24):241102.
PMID: 27367378
On September 14, 2015, the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected a gravitational-wave transient (GW150914); we characterize the properties of the source and its parameters. The data around the time...
23.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2016 Jun;
116(22):221101.
PMID: 27314708
The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to witness the final merger...
24.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2016 Apr;
116(13):131103.
PMID: 27081966
Following a major upgrade, the two advanced detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) held their first observation run between September 2015 and January 2016. With a strain sensitivity...
25.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2016 Apr;
116(13):131102.
PMID: 27081965
The LIGO detection of the gravitational wave transient GW150914, from the inspiral and merger of two black holes with masses ≳30M_{⊙}, suggests a population of binary black holes with relatively...
26.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2016 Feb;
116(6):061102.
PMID: 26918975
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35...
27.
Aasi J, Abbott B, Abbott R, Abbott T, Abernathy M, Accadia T, et al.
Phys Rev Lett
. 2014 Dec;
113(23):231101.
PMID: 25526109
Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history of the...
28.
Aasi J, Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, et al.
Phys Rev Lett
. 2014 Jul;
113(1):011102.
PMID: 25032916
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science...
29.
Aasi J, Abadie J, Abbott B, Abbott R, Abbott T, Abernathy M, et al.
Phys Rev Lett
. 2014 Apr;
112(13):131101.
PMID: 24745400
Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In...