Dr. Michael Pürrer
Dr. Michael Pürrer
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Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model
B.~P. Abbott
,
R. Abbott
,
T.~D. Abbott
,
M.~R. Abernathy
,
F. Acernese
,
K. Ackley
,
C. Adams
,
T. Adams
,
P. Addesso
,
et al
October 2016
Cite
DOI
Type
Journal article
Publication
Physical Review X
"General Relativity and Quantum Cosmology"
"Astrophysics - High Energy Astrophysical Phenomena"
Related
Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
Supplement: “Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914” (2016, ApJL, 826, L13)
Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
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