Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data

J. Aasi; B.P. Abbott; R. Abbott; T. Abbott; M.R. Abernathy; T. Accadia; F. Acernese; K. Ackley; C. Adams; T. Adams; P. Addesso; R.X. Adhikari; C. Affeldt; M. Agathos; N. Aggarwal; O.D. Aguiar; A. Ain; P. Ajith; A. Alemic; B. Allen; A. Allocca; D. Amariutei; M. Andersen; R. Anderson; S.B. Anderson; W.G. Anderson; K. Arai; M.C. Araya; C. Arceneaux; J. Areeda; S.M. Aston; P. Astone; P. Aufmuth; C. Aulbert; L. Austin; B.E. Aylott; S. Babak; P.T. Baker; G. Ballardin; S.W. Ballmer; J.C. Barayoga; M. Barbet; B.C. Barish; D. Barker; F. Barone; B. Barr; L. Barsotti; M. Barsuglia; M.A. Barton; I. Bartos; R. Bassiri; A. Basti; J.C. Batch; J. Bauchrowitz; Th. S. Bauer; B. Behnke; M. Bejger; M.G. Beker; C. Belczynski; A.S. Bell; C. Bell; G. Bergmann; D. Bersanetti; A. Bertolini; J. Betzwieser; P.T. Beyersdorf; I.A. Bilenko; G. Billingsley; J. Birch; S. Biscans; M. Bitossi; M.A. Bizouard; E. Black; J.K. Blackburn; L. Blackburn; D. Blair; S. Bloemen; M. Blom; O. Bock; T.P. Bodiya; M. Boer; G. Bogaert; C. Bogan; C. Bond; F. Bondu; L. Bonelli; R. Bonnand; R. Bork; M. Born; V. Boschi; Sukanta Bose; L. Bosi; C. Bradaschia; P.R. Brady; V.B. Braginsky; M. Branchesi; J.E. Brau; T. Briant; D.O. Bridges; A. Brillet; M. Brinkmann; V. Brisson; A.F. Brooks; D.A. Brown; D.D. Brown; F. Brückner; S. Buchman; T. Bulik; H.J. Bulten; A. Buonanno; R. Burman; D. Buskulic; C. Buy; L. Cadonati; G. Cagnoli; J. Calderón Bustillo; E. Calloni; J.B. Camp; P. Campsie; K.C. Cannon; B. Canuel; J. Cao; C.D. Capano; F. Carbognani; L. Carbone; S. Caride; A. Castiglia; S. Caudill; M. Cavaglià; F. Cavalier; R. Cavalieri; C. Celerier; G. Cella; C. Cepeda; E. Cesarini; R. Chakraborty; T. Chalermsongsak; S.J. Chamberlin; S. Chao; P. Charlton; E. Chassande-Mottin; X. Chen; Y. Chen; A. Chincarini; A. Chiummo; H.S. Cho; J. Chow; N. Christensen; Q. Chu; S.S.Y. Chua; S. Chung; G. Ciani; F. Clara; J.A. Clark; F. Cleva; E. Coccia; P.-F. Cohadon; A. Colla; C. Collette; M. Colombini; L. Cominsky; M. Constancio; A. Conte; D. Cook; T.R. Corbitt; M. Cordier; N. Cornish; A. Corpuz; A. Corsi; C.A. Costa; M.W. Coughlin; S. Coughlin; J.-P. Coulon; S. Countryman; P. Couvares; D.M. Coward; M. Cowart; D.C. Coyne; R. Coyne; K. Craig; J.D.E. Creighton; S.G. Crowder; A. Cumming; L. Cunningham; E. Cuoco; K. Dahl; T. Dal Canton; M. Damjanic; S.L. Danilishin; S. D''Antonio; K. Danzmann; V. Dattilo; H. Daveloza; M. Davier; G.S. Davies; E.J. Daw; R. Day; T. Dayanga; G. Debreczeni; J. Degallaix; S. Deléglise; W. Del Pozzo; T. Denker; T. Dent; H. Dereli; V. Dergachev; R. De Rosa; R.T. Derosa; R. Desalvo; S. Dhurandhar; M. Díaz; L. Di Fiore; A. Di Lieto; I. Di Palma; A. Di Virgilio; A. Donath; F. Donovan; K.L. Dooley; S. Doravari; S. Dossa; R. Douglas; T.P. Downes; M. Drago; R.W.P. Drever; J.C. Driggers; Z. Du; S. Dwyer; T. Eberle; T. Edo; M. Edwards; A. Effler; H. Eggenstein; P. Ehrens; J. Eichholz; S.S. Eikenberry; G. Endroczi; R. Essick; T. Etzel; M. Evans; T. Evans; M. Factourovich; V. Fafone; S. Fairhurst; Q. Fang; S. Farinon; B. Farr; W.M. Farr; M. Favata; H. Fehrmann; M.M. Fejer; D. Feldbaum; F. Feroz; I. Ferrante; F. Ferrini; F. Fidecaro; L.S. Finn; I. Fiori; R.P. Fisher; R. Flaminio; J.-D. Fournier; S. Franco; S. Frasca; F. Frasconi; M. Frede; Z. Frei; A. Freise; R. Frey; T.T. Fricke; P. Fritschel; V.V. Frolov; P. Fulda; M. Fyffe; J. Gair; L. Gammaitoni; S. Gaonkar; F. Garufi; N. Gehrels; G. Gemme; E. Genin; A. Gennai; S. Ghosh; J.A. Giaime; K.D. Giardina; A. Giazotto; C. Gill; J. Gleason; E. Goetz; R. Goetz; L. Gondan; G. González; N. Gordon; M.L. Gorodetsky; S. Gossan; S. Goßler; R. Gouaty; C. Gräf; P.B. Graff; M. Granata; A. Grant; S. Gras; C. Gray; R.J.S. Greenhalgh; A.M. Gretarsson; P. Groot; H. Grote; K. Grover; S. Grunewald; G.M. Guidi; C. Guido; K. Gushwa; E.K. Gustafson; R. Gustafson; D. Hammer; G. Hammond; M. Hanke; J. Hanks; C. Hanna; J. Hanson; J. Harms; G.M. Harry; I.W. Harry; E.D. Harstad; M. Hart; M.T. Hartman; C.-J. Haster; K. Haughian; A. Heidmann; M. Heintze; H. Heitmann; P. Hello; G. Hemming; M. Hendry; I.S. Heng; A.W. Heptonstall; M. Heurs; M. Hewitson; S. Hild; D. Hoak; K.A. Hodge; K. Holt; S. Hooper; P. Hopkins; D.J. Hosken; J. Hough; E.J. Howell; Y. Hu; E. Huerta; B. Hughey; S. Husa; S.H. Huttner; M. Huynh; T. Huynh-Dinh; D.R. Ingram; R. Inta; T. Isogai; A. Ivanov; B.R. Iyer; K. Izumi; M. Jacobson; E. James; H. Jang; P. Jaranowski; Y. Ji; F. Jiménez-Forteza; W.W. Johnson; D.I. Jones; R. Jones; R.J.G. Jonker; L. Ju; P. Kalmus; V. Kalogera; S. Kandhasamy; G. Kang; J.B. Kanner; J. Karlen; M. Kasprzack; E. Katsavounidis; W. Katzman; H. Kaufer; K. Kawabe; F. Kawazoe; F. Kéfélian; G.M. Keiser; D. Keitel; D.B. Kelley; W. Kells; A. Khalaidovski; F.Y. Khalili; E.A. Khazanov; C. Kim; K. Kim; N. Kim; N.G. Kim; Y.-M. Kim; E.J. King; P.J. King; D.L. Kinzel; J.S. Kissel; S. Klimenko; J. Kline; S. Koehlenbeck; K. Kokeyama; V. Kondrashov; S. Koranda; W.Z. Korth; I. Kowalska; D.B. Kozak; A. Kremin; V. Kringel; A. Królak; G. Kuehn; A. Kumar; P. Kumar; R. Kumar; L. Kuo; A. Kutynia; P. Kwee; M. Landry; B. Lantz; S. Larson; P.D. Lasky; C. Lawrie; A. Lazzarini; C. Lazzaro; P. Leaci; S. Leavey; E.O. Lebigot; C.-H. Lee; H.K. Lee; H.M. Lee; J. Lee; M. Leonardi; J.R. Leong; A. Le Roux; N. Leroy; N. Letendre; Y. Levin; B. Levine; J. Lewis; T.G.F. Li; K. Libbrecht; A. Libson; A.C. Lin; T.B. Littenberg; V. Litvine; N.A. Lockerbie; V. Lockett; D. Lodhia; K. Loew; J. Logue; A.L. Lombardi; M. Lorenzini; V. Loriette; M. Lormand; G. Losurdo; J. Lough; M.J. Lubinski; H. Lück; E. Luijten; A.P. Lundgren; R. Lynch; Y. Ma; J. Macarthur; E.P. Macdonald; T. Macdonald; B. Machenschalk; M. Macinnis; D.M. Macleod; F. Magana-Sandoval; M. Mageswaran; C. Maglione; K. Mailand; E. Majorana; I. Maksimovic; V. Malvezzi; N. Man; G.M. Manca; I. Mandel; V. Mandic; V. Mangano; N. Mangini; M. Mantovani; F. Marchesoni; F. Marion; S. Márka; Z. Márka; A. Markosyan; E. Maros; J. Marque; F. Martelli; I.W. Martin; R.M. Martin; L. Martinelli; D. Martynov; J.N. Marx; K. Mason; A. 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doi:10.1103/PhysRevLett.113.231101

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Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data

J. Aasi, B.P. Abbott, R. Abbott, T. Abbott, M.R. Abernathy, T. Accadia, F. Acernese, K. Ackley, C. Adams, T. Adams, …

Physical Review Letters, Vol.113(23), 231101

02/12/2014

DOI: https://doi.org/10.1103/PhysRevLett.113.231101

Abstract

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 Universe that is unavailable through standard electromagnetic observations, making its study of fundamental importance to understanding the evolution of the Universe. We carry out a search for the stochastic background with the latest data from the LIGO and Virgo detectors. Consistent with predictions from most stochastic gravitational-wave background models, the data display no evidence of a stochastic gravitational-wave signal. Assuming a gravitational-wave spectrum of ?GW(f)=??(f/fref)?, we place 95% confidence level upper limits on the energy density of the background in each of four frequency bands spanning 41.5-1726 Hz. In the frequency band of 41.5-169.25 Hz for a spectral index of ?=0, we constrain the energy density of the stochastic background to be ?GW(f)<5.6×10-6. For the 600-1000 Hz band, ?GW(f)<0.14(f/900Hz)3, a factor of 2.5 lower than the best previously reported upper limits. We find ?GW(f)<1.8×10-4 using a spectral index of zero for 170-600 Hz and ?GW(f)<1.0(f/1300Hz)3 for 1000-1726 Hz, bands in which no previous direct limits have been placed. The limits in these four bands are the lowest direct measurements to date on the stochastic background. We discuss the implications of these results in light of the recent claim by the BICEP2 experiment of the possible evidence for inflationary gravitational waves.

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Title: Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data
Creators - without role: J. Aasi - California Institute of Technology
B.P. Abbott - California Institute of Technology
R. Abbott - California Institute of Technology
T. Abbott - Louisiana State University
M.R. Abernathy - California Institute of Technology
T. Accadia - Centre National de la Recherche Scientifique
F. Acernese - University of Salerno
K. Ackley - University of Florida
C. Adams - LIGO Scientific Collaboration
T. Adams - Cardiff University
P. Addesso - University of Salerno
R.X. Adhikari - California Institute of Technology
C. Affeldt - Max Planck Institute for Gravitational Physics
M. Agathos - National Institute for Subatomic Physics
N. Aggarwal - Massachusetts Institute of Technology
O.D. Aguiar - Instituto Nacional de Pesquisas Espaciais
A. Ain - Inter-University Centre for Astronomy and Astrophysics
P. Ajith - Tata Institute of Fundamental Research
A. Alemic - Syracuse University
B. Allen - Leibniz University Hannover
A. Allocca - University of Siena
D. Amariutei - University of Florida
M. Andersen - Stanford University
R. Anderson - California Institute of Technology
S.B. Anderson - California Institute of Technology
W.G. Anderson - University of Wisconsin–Milwaukee
K. Arai - California Institute of Technology
M.C. Araya - California Institute of Technology
C. Arceneaux - University of Mississippi
J. Areeda - California State University, Fullerton
S.M. Aston - LIGO Scientific Collaboration
P. Astone - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
P. Aufmuth - Leibniz University Hannover
C. Aulbert - Max Planck Institute for Gravitational Physics
L. Austin - California Institute of Technology
B.E. Aylott - University of Birmingham
S. Babak - Max Planck Institute for Gravitational Physics
P.T. Baker - Montana State University
G. Ballardin - European Gravitational Observatory
S.W. Ballmer - Syracuse University
J.C. Barayoga - California Institute of Technology
M. Barbet - University of Florida
B.C. Barish - California Institute of Technology
D. Barker - LIGO - Hanford Observatory
F. Barone - University of Salerno
B. Barr - University of Glasgow
L. Barsotti - Massachusetts Institute of Technology
M. Barsuglia - Centre National de la Recherche Scientifique
M.A. Barton - LIGO - Hanford Observatory
I. Bartos - Columbia University
R. Bassiri - Stanford University
A. Basti - University of Pisa
J.C. Batch - LIGO - Hanford Observatory
J. Bauchrowitz - Max Planck Institute for Gravitational Physics
Th. S. Bauer - National Institute for Subatomic Physics
B. Behnke - Max Planck Institute for Gravitational Physics
M. Bejger - CAMK-PAN
M.G. Beker - National Institute for Subatomic Physics
C. Belczynski - Astronomical Observatory
A.S. Bell - University of Glasgow
C. Bell - University of Glasgow
G. Bergmann - Max Planck Institute for Gravitational Physics
D. Bersanetti - Istituto Nazionale di Fisica Nucleare, Sezione di Genova
A. Bertolini - National Institute for Subatomic Physics
J. Betzwieser - LIGO Scientific Collaboration
P.T. Beyersdorf - San Jose State University
I.A. Bilenko - Lomonosov Moscow State University
G. Billingsley - California Institute of Technology
J. Birch - LIGO Scientific Collaboration
S. Biscans - Massachusetts Institute of Technology
M. Bitossi - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
M.A. Bizouard - Université Paris-Sud
E. Black - California Institute of Technology
J.K. Blackburn - California Institute of Technology
L. Blackburn - Goddard Space Flight Center
D. Blair - The University of Western Australia
S. Bloemen - Radboud University Nijmegen
M. Blom - National Institute for Subatomic Physics
O. Bock - Max Planck Institute for Gravitational Physics
T.P. Bodiya - Massachusetts Institute of Technology
M. Boer - Centre National de la Recherche Scientifique
G. Bogaert - Centre National de la Recherche Scientifique
C. Bogan - Max Planck Institute for Gravitational Physics
C. Bond - University of Birmingham
F. Bondu - Université de Rennes
L. Bonelli - University of Pisa
R. Bonnand - Université Claude Bernard Lyon 1
R. Bork - California Institute of Technology
M. Born - Max Planck Institute for Gravitational Physics
V. Boschi - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Sukanta Bose - Inter-University Centre for Astronomy and Astrophysics
L. Bosi - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
C. Bradaschia - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
P.R. Brady - University of Wisconsin–Milwaukee
V.B. Braginsky - Lomonosov Moscow State University
M. Branchesi - University of Urbino
J.E. Brau - University of Oregon
T. Briant - Centre National de la Recherche Scientifique
D.O. Bridges - LIGO Scientific Collaboration
A. Brillet - Centre National de la Recherche Scientifique
M. Brinkmann - Max Planck Institute for Gravitational Physics
V. Brisson - Université Paris-Sud
A.F. Brooks - California Institute of Technology
D.A. Brown - Syracuse University
D.D. Brown - Syracuse University
F. Brückner - University of Birmingham
S. Buchman - Stanford University
T. Bulik - University of Warsaw
H.J. Bulten - National Institute for Subatomic Physics
A. Buonanno - University of Maryland, College Park
R. Burman - The University of Western Australia
D. Buskulic - Centre National de la Recherche Scientifique
C. Buy - Centre National de la Recherche Scientifique
L. Cadonati - University of Massachusetts Amherst
G. Cagnoli - Université Claude Bernard Lyon 1
J. Calderón Bustillo - Universitat de les Illes Balears
E. Calloni - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
J.B. Camp - Goddard Space Flight Center
P. Campsie - University of Glasgow
K.C. Cannon - University of Toronto
B. Canuel - European Gravitational Observatory
J. Cao - Tsinghua University
C.D. Capano - University of Maryland, College Park
F. Carbognani - European Gravitational Observatory
L. Carbone - University of Birmingham
S. Caride - University of Michigan
A. Castiglia - Rochester Institute of Technology
S. Caudill - University of Wisconsin–Milwaukee
M. Cavaglià - University of Mississippi
F. Cavalier - Université Paris-Sud
R. Cavalieri - European Gravitational Observatory
C. Celerier - Stanford University
G. Cella - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
C. Cepeda - California Institute of Technology
E. Cesarini - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
R. Chakraborty - California Institute of Technology
T. Chalermsongsak - California Institute of Technology
S.J. Chamberlin - University of Wisconsin–Milwaukee
S. Chao - National Tsing Hua University
P. Charlton - Charles Sturt University
E. Chassande-Mottin - Sorbonne Paris Cité
X. Chen - The University of Western Australia
Y. Chen - California Institute of Technology
A. Chincarini - Istituto Nazionale di Fisica Nucleare, Sezione di Genova
A. Chiummo - European Gravitational Observatory
H.S. Cho - Pusan National University
J. Chow - Australian National University
N. Christensen - Carleton College
Q. Chu - The University of Western Australia
S.S.Y. Chua - Australian National University
S. Chung - The University of Western Australia
G. Ciani - University of Florida
F. Clara - LIGO - Hanford Observatory
J.A. Clark - University of Massachusetts Amherst
F. Cleva - Centre National de la Recherche Scientifique
E. Coccia - University of Rome Tor Vergata
P.-F. Cohadon - Laboratoire Kastler Brossel
A. Colla - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
C. Collette - University of Brussels
M. Colombini - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
L. Cominsky - Sonoma State University
M. Constancio - Instituto Nacional de Pesquisas Espaciais
A. Conte - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
D. Cook - LIGO - Hanford Observatory
T.R. Corbitt - Louisiana State University
M. Cordier - San Jose State University
N. Cornish - Montana State University
A. Corpuz - Embry–Riddle Aeronautical University
A. Corsi - George Washington University
C.A. Costa - Instituto Nacional de Pesquisas Espaciais
M.W. Coughlin - University of Cambridge
S. Coughlin - Northwestern University
J.-P. Coulon - Observatoire de la Côte d’Azur
S. Countryman - Columbia University
P. Couvares - Syracuse University
D.M. Coward - The University of Western Australia
M. Cowart - LIGO Scientific Collaboration
D.C. Coyne - California Institute of Technology
R. Coyne - George Washington University
K. Craig - University of Glasgow
J.D.E. Creighton - University of Wisconsin–Milwaukee
S.G. Crowder - University of Minnesota
A. Cumming - University of Glasgow
L. Cunningham - University of Glasgow
E. Cuoco - European Gravitational Observatory
K. Dahl - Max Planck Institute for Gravitational Physics
T. Dal Canton - Max Planck Institute for Gravitational Physics
M. Damjanic - Max Planck Institute for Gravitational Physics
S.L. Danilishin - The University of Western Australia
S. D''Antonio - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
K. Danzmann - Leibniz University Hannover
V. Dattilo - European Gravitational Observatory
H. Daveloza - Brownsville Public Library
M. Davier - Université Paris-Sud
G.S. Davies - University of Glasgow
E.J. Daw - University of Sheffield
R. Day - European Gravitational Observatory
T. Dayanga - Washington State University
G. Debreczeni - HUN-REN Wigner Research Centre for Physics
J. Degallaix - Centre National de la Recherche Scientifique
S. Deléglise - Centre National de la Recherche Scientifique
W. Del Pozzo - National Institute for Subatomic Physics
T. Denker - Max Planck Institute for Gravitational Physics
T. Dent - Max Planck Institute for Gravitational Physics
H. Dereli - Centre National de la Recherche Scientifique
V. Dergachev - California Institute of Technology
R. De Rosa - Louisiana State University
R.T. Derosa - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
R. Desalvo - University of Sannio
S. Dhurandhar - Inter-University Centre for Astronomy and Astrophysics
M. Díaz - Brownsville Public Library
L. Di Fiore - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
A. Di Lieto - University of Pisa
I. Di Palma - Max Planck Institute for Gravitational Physics
A. Di Virgilio - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
A. Donath - Max Planck Institute for Gravitational Physics
F. Donovan - Massachusetts Institute of Technology
K.L. Dooley - Max Planck Institute for Gravitational Physics
S. Doravari - LIGO Scientific Collaboration
S. Dossa - Carleton College
R. Douglas - University of Glasgow
T.P. Downes - University of Wisconsin–Milwaukee
M. Drago - University of Trento
R.W.P. Drever - California Institute of Technology
J.C. Driggers - California Institute of Technology
Z. Du - Tsinghua University
S. Dwyer - LIGO - Hanford Observatory
T. Eberle - Max Planck Institute for Gravitational Physics
T. Edo - University of Sheffield
M. Edwards - Cardiff University
A. Effler - Louisiana State University
H. Eggenstein - Max Planck Institute for Gravitational Physics
P. Ehrens - California Institute of Technology
J. Eichholz - University of Florida
S.S. Eikenberry - University of Florida
G. Endroczi - HUN-REN Wigner Research Centre for Physics
R. Essick - Massachusetts Institute of Technology
T. Etzel - California Institute of Technology
M. Evans - Massachusetts Institute of Technology
T. Evans - LIGO Scientific Collaboration
M. Factourovich - Columbia University
V. Fafone - University of Rome Tor Vergata
S. Fairhurst - Cardiff University
Q. Fang - The University of Western Australia
S. Farinon - Istituto Nazionale di Fisica Nucleare, Sezione di Genova
B. Farr - Northwestern University
W.M. Farr - University of Birmingham
M. Favata - Montclair State University
H. Fehrmann - Max Planck Institute for Gravitational Physics
M.M. Fejer - Stanford University
D. Feldbaum - LIGO Scientific Collaboration
F. Feroz - University of Cambridge
I. Ferrante - University of Pisa
F. Ferrini - European Gravitational Observatory
F. Fidecaro - University of Pisa
L.S. Finn - Pennsylvania State University
I. Fiori - European Gravitational Observatory
R.P. Fisher - Syracuse University
R. Flaminio - Centre National de la Recherche Scientifique
J.-D. Fournier - Observatoire de la Côte d’Azur
S. Franco - Université Paris-Sud
S. Frasca - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
F. Frasconi - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
M. Frede - Max Planck Institute for Gravitational Physics
Z. Frei - Eötvös Loránd University
A. Freise - University of Birmingham
R. Frey - University of Oregon
T.T. Fricke - Max Planck Institute for Gravitational Physics
P. Fritschel - Massachusetts Institute of Technology
V.V. Frolov - LIGO Scientific Collaboration
P. Fulda - University of Florida
M. Fyffe - LIGO Scientific Collaboration
J. Gair - University of Cambridge
L. Gammaitoni - University of Perugia
S. Gaonkar - Inter-University Centre for Astronomy and Astrophysics
F. Garufi - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
N. Gehrels - Goddard Space Flight Center
G. Gemme - Istituto Nazionale di Fisica Nucleare, Sezione di Genova
E. Genin - European Gravitational Observatory
A. Gennai - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
S. Ghosh - Radboud University Nijmegen
J.A. Giaime - LIGO Scientific Collaboration
K.D. Giardina - LIGO Scientific Collaboration
A. Giazotto - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
C. Gill - University of Glasgow
J. Gleason - University of Florida
E. Goetz - University of Florida
R. Goetz - University of Florida
L. Gondan - Eötvös Loránd University
G. González - Louisiana State University
N. Gordon - University of Glasgow
M.L. Gorodetsky - Lomonosov Moscow State University
S. Gossan - California Institute of Technology
S. Goßler - Max Planck Institute for Gravitational Physics
R. Gouaty - Laboratoire d’Annecy de Physique des Particules
C. Gräf - University of Glasgow
P.B. Graff - Goddard Space Flight Center
M. Granata - Centre National de la Recherche Scientifique
A. Grant - University of Glasgow
S. Gras - Massachusetts Institute of Technology
C. Gray - LIGO - Hanford Observatory
R.J.S. Greenhalgh - Rutherford Appleton Laboratory
A.M. Gretarsson - Embry–Riddle Aeronautical University
P. Groot - Radboud University Nijmegen
H. Grote - Max Planck Institute for Gravitational Physics
K. Grover - University of Birmingham
S. Grunewald - Max Planck Institute for Gravitational Physics
G.M. Guidi - University of Urbino
C. Guido - LIGO Scientific Collaboration
K. Gushwa - California Institute of Technology
E.K. Gustafson - California Institute of Technology
R. Gustafson - University of Michigan
D. Hammer - University of Wisconsin–Milwaukee
G. Hammond - University of Glasgow
M. Hanke - Max Planck Institute for Gravitational Physics
J. Hanks - LIGO - Hanford Observatory
C. Hanna - Perimeter Institute
J. Hanson - LIGO Scientific Collaboration
J. Harms - California Institute of Technology
G.M. Harry - American University
I.W. Harry - American University
E.D. Harstad - University of Oregon
M. Hart - University of Glasgow
M.T. Hartman - University of Florida
C.-J. Haster - University of Birmingham
K. Haughian - University of Glasgow
A. Heidmann - Centre National de la Recherche Scientifique
M. Heintze - LIGO Scientific Collaboration
H. Heitmann - Centre National de la Recherche Scientifique
P. Hello - Université Paris-Sud
G. Hemming - European Gravitational Observatory
M. Hendry - University of Glasgow
I.S. Heng - University of Glasgow
A.W. Heptonstall - California Institute of Technology
M. Heurs - Max Planck Institute for Gravitational Physics
M. Hewitson - Max Planck Institute for Gravitational Physics
S. Hild - University of Glasgow
D. Hoak - University of Massachusetts Amherst
K.A. Hodge - California Institute of Technology
K. Holt - LIGO Scientific Collaboration
S. Hooper - The University of Western Australia
P. Hopkins - Cardiff University
D.J. Hosken - The University of Adelaide
J. Hough - University of Glasgow
E.J. Howell - The University of Western Australia
Y. Hu - University of Glasgow
E. Huerta - Syracuse University
B. Hughey - Embry–Riddle Aeronautical University
S. Husa - Universitat de les Illes Balears
S.H. Huttner - University of Glasgow
M. Huynh - University of Wisconsin–Milwaukee
T. Huynh-Dinh - LIGO - Livingston Observatory
D.R. Ingram - LIGO - Hanford Observatory
R. Inta - Pennsylvania State University
T. Isogai - Massachusetts Institute of Technology
A. Ivanov - California Institute of Technology
B.R. Iyer - Raman Research Institute
K. Izumi - LIGO - Hanford Observatory
M. Jacobson - California Institute of Technology
E. James - California Institute of Technology
H. Jang - Korea Institute of Science & Technology Information
P. Jaranowski - Biał Ystok University
Y. Ji - Tsinghua University
F. Jiménez-Forteza - Universitat de les Illes Balears
W.W. Johnson - Louisiana State University
D.I. Jones - University of Southampton
R. Jones - University of Glasgow
R.J.G. Jonker - National Institute for Subatomic Physics
L. Ju - The University of Western Australia
P. Kalmus - California Institute of Technology
V. Kalogera - Northwestern University
S. Kandhasamy - University of Mississippi
G. Kang - Korea Institute of Science & Technology Information
J.B. Kanner - California Institute of Technology
J. Karlen - University of Massachusetts Amherst
M. Kasprzack - Université Paris-Sud
E. Katsavounidis - Massachusetts Institute of Technology
W. Katzman - LIGO Scientific Collaboration
H. Kaufer - Leibniz University Hannover
K. Kawabe - LIGO - Hanford Observatory
F. Kawazoe - Max Planck Institute for Gravitational Physics
F. Kéfélian - Centre National de la Recherche Scientifique
G.M. Keiser - Stanford University
D. Keitel - Max Planck Institute for Gravitational Physics
D.B. Kelley - Syracuse University
W. Kells - California Institute of Technology
A. Khalaidovski - Max Planck Institute for Gravitational Physics
F.Y. Khalili - Lomonosov Moscow State University
E.A. Khazanov - Institute of Applied Physics
C. Kim - Seoul National University
K. Kim - Hanyang University
N. Kim - Stanford University
N.G. Kim - Stanford University
Y.-M. Kim - Pusan National University
E.J. King - The University of Adelaide
P.J. King - California Institute of Technology
D.L. Kinzel - LIGO Scientific Collaboration
J.S. Kissel - LIGO - Hanford Observatory
S. Klimenko - University of Florida
J. Kline - University of Wisconsin–Milwaukee
S. Koehlenbeck - Max Planck Institute for Gravitational Physics
K. Kokeyama - Louisiana State University
V. Kondrashov - California Institute of Technology
S. Koranda - University of Wisconsin–Milwaukee
W.Z. Korth - California Institute of Technology
I. Kowalska - University of Warsaw
D.B. Kozak - California Institute of Technology
A. Kremin - University of Minnesota
V. Kringel - Max Planck Institute for Gravitational Physics
A. Królak - Institute of Mathematics
G. Kuehn - Max Planck Institute for Gravitational Physics
A. Kumar - Institute for Plasma Research
P. Kumar - Syracuse University
R. Kumar - University of Glasgow
L. Kuo - National Tsing Hua University
A. Kutynia - National Centre for Nuclear Research
P. Kwee - Massachusetts Institute of Technology
M. Landry - LIGO - Hanford Observatory
B. Lantz - Stanford University
S. Larson - Northwestern University
P.D. Lasky - The University of Melbourne
C. Lawrie - University of Glasgow
A. Lazzarini - California Institute of Technology
C. Lazzaro - INFN Sezione di Padova
P. Leaci - Max Planck Institute for Gravitational Physics
S. Leavey - University of Glasgow
E.O. Lebigot - Tsinghua University
C.-H. Lee - Pusan National University
H.K. Lee - Hanyang University
H.M. Lee - Seoul National University
J. Lee - Massachusetts Institute of Technology
M. Leonardi - University of Trento
J.R. Leong - Max Planck Institute for Gravitational Physics
A. Le Roux - LIGO Scientific Collaboration
N. Leroy - Université Paris-Sud
N. Letendre - Laboratoire d’Annecy de Physique des Particules
Y. Levin - Monash University
B. Levine - LIGO - Hanford Observatory
J. Lewis - California Institute of Technology
T.G.F. Li - California Institute of Technology
K. Libbrecht - California Institute of Technology
A. Libson - Massachusetts Institute of Technology
A.C. Lin - Stanford University
T.B. Littenberg - Northwestern University
V. Litvine - California Institute of Technology
N.A. Lockerbie - University of Strathclyde
V. Lockett - California State University, Fullerton
D. Lodhia - University of Birmingham
K. Loew - Embry–Riddle Aeronautical University
J. Logue - University of Glasgow
A.L. Lombardi - University of Massachusetts Amherst
M. Lorenzini - University of Rome Tor Vergata
V. Loriette - ESPCI Paris
M. Lormand - LIGO Scientific Collaboration
G. Losurdo - Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
J. Lough - Syracuse University
M.J. Lubinski - LIGO - Hanford Observatory
H. Lück - Max Planck Institute for Gravitational Physics
E. Luijten - Northwestern University
A.P. Lundgren - Max Planck Institute for Gravitational Physics
R. Lynch - Massachusetts Institute of Technology
Y. Ma - The University of Western Australia
J. Macarthur - University of Glasgow
E.P. Macdonald - Cardiff University
T. Macdonald - Stanford University
B. Machenschalk - Max Planck Institute for Gravitational Physics
M. Macinnis - Massachusetts Institute of Technology
D.M. Macleod - Louisiana State University
F. Magana-Sandoval - Syracuse University
M. Mageswaran - California Institute of Technology
C. Maglione - Argentinian Gravitational Wave Group , Cordoba , Cordoba
K. Mailand - California Institute of Technology
E. Majorana - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
I. Maksimovic - Centre National de la Recherche Scientifique
V. Malvezzi - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
N. Man - Centre National de la Recherche Scientifique
G.M. Manca - Max Planck Institute for Gravitational Physics
I. Mandel - University of Birmingham
V. Mandic - University of Minnesota
V. Mangano - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
N. Mangini - University of Massachusetts Amherst
M. Mantovani - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
F. Marchesoni - Università di Camerino
F. Marion - Institut National de Physique Nucléaire et de Physique des Particules
S. Márka - Columbia University
Z. Márka - Columbia University
A. Markosyan - Stanford University
E. Maros - California Institute of Technology
J. Marque - European Gravitational Observatory
F. Martelli - University of Urbino
I.W. Martin - University of Glasgow
R.M. Martin - University of Florida
L. Martinelli - Centre National de la Recherche Scientifique
D. Martynov - LIGO - California Institute of Technology
J.N. Marx - California Institute of Technology
K. Mason - Massachusetts Institute of Technology
A. Masserot - Laboratoire d’Annecy de Physique des Particules
T.J. Massinger - Syracuse University
F. Matichard - Massachusetts Institute of Technology
L. Matone - Columbia University
R.A. Matzner - The University of Texas at Austin
N. Mavalvala - Massachusetts Institute of Technology
N. Mazumder - Indian Institute of Science Education and Research Thiruvananthapuram
G. Mazzolo - Max Planck Institute for Gravitational Physics
R. McCarthy - LIGO - Hanford Observatory
D.E. McClelland - Australian National University
S.C. McGuire - Southern University and Agricultural and Mechanical College
G. McIntyre - California Institute of Technology
J. McIver - University of Massachusetts Amherst
K. McLin - Sonoma State University
D. Meacher - Centre National de la Recherche Scientifique
G.D. Meadors - University of Michigan
M. Mehmet - Max Planck Institute for Gravitational Physics
J. Meidam - National Institute for Subatomic Physics
M. Meinders - Leibniz University Hannover
A. Melatos - The University of Melbourne
G. Mendell - LIGO - Hanford Observatory
R.A. Mercer - University of Wisconsin–Milwaukee
S. Meshkov - California Institute of Technology
C. Messenger - University of Glasgow
P. Meyers - University of Minnesota
H. Miao - California Institute of Technology
C. Michel - Laboratoire des Matériaux Avancés
E.E. Mikhailov - College of William and Mary
L. Milano - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
S. Milde - Max Planck Institute for Gravitational Physics
J. Miller - Massachusetts Institute of Technology
Y. Minenkov - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
C.M.F. Mingarelli - University of Birmingham
C. Mishra - Indian Institute of Science Education and Research Thiruvananthapuram
S. Mitra - Inter-University Centre for Astronomy and Astrophysics
V.P. Mitrofanov - Lomonosov Moscow State University
G. Mitselmakher - University of Florida
R. Mittleman - Massachusetts Institute of Technology
B. Moe - University of Wisconsin–Milwaukee
P. Moesta - California Institute of Technology
M. Mohan - European Gravitational Observatory
S.R.P. Mohapatra - Rochester Institute of Technology
D. Moraru - LIGO - Hanford Observatory
G. Moreno - LIGO - Hanford Observatory
N. Morgado - Université Claude Bernard Lyon 1
S.R. Morriss - Brownsville Public Library
K. Mossavi - Max Planck Institute for Gravitational Physics
B. Mours - Laboratoire d’Annecy de Physique des Particules
C.M. Mow-Lowry - Max Planck Institute for Gravitational Physics
C.L. Mueller - University of Florida
G. Mueller - University of Florida
S. Mukherjee - Brownsville Public Library
A. Mullavey - Louisiana State University
J. Munch - The University of Adelaide
D. Murphy - Columbia University
P.G. Murray - University of Glasgow
A. Mytidis - University of Florida
M.F. Nagy - HUN-REN Wigner Research Centre for Physics
D. Nanda Kumar - University of Florida
I. Nardecchia - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
L. Naticchioni - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
R.K. Nayak - Indian Institute of Science Education and Research Kolkata
V. Necula - University of Florida
G. Nelemans - Radboud University Nijmegen
I. Neri - University of Perugia
M. Neri - Istituto Nazionale di Fisica Nucleare, Sezione di Genova
G. Newton - University of Glasgow
T. Nguyen - Australian National University
A. Nitz - Syracuse University
F. Nocera - European Gravitational Observatory
D. Nolting - LIGO Scientific Collaboration
M.E.N. Normandin - Brownsville Public Library
L.K. Nuttall - University of Wisconsin–Milwaukee
E. Ochsner - University of Wisconsin–Milwaukee
J. O''Dell - Rutherford Appleton Laboratory
E. Oelker - Massachusetts Institute of Technology
J.J. Oh - National Institute for Mathematical Sciences
S.H. Oh - National Institute for Mathematical Sciences
F. Ohme - Cardiff University
P. Oppermann - Max Planck Institute for Gravitational Physics
B. O''Reilly - LIGO - Livingston Observatory
R. O''Shaughnessy - University of Wisconsin–Milwaukee
C. Osthelder - California Institute of Technology
D.J. Ottaway - The University of Adelaide
R.S. Ottens - University of Florida
H. Overmier - LIGO Scientific Collaboration
B.J. Owen - Pennsylvania State University
C. Padilla - California State University, Fullerton
A. Pai - Indian Institute of Science Education and Research Thiruvananthapuram
O. Palashov - Institute of Applied Physics
C. Palomba - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
H. Pan - National Tsing Hua University
Y. Pan - University of Maryland, College Park
C. Pankow - University of Wisconsin–Milwaukee
F. Paoletti - European Gravitational Observatory
R. Paoletti - University of Siena
H. Paris - LIGO - Hanford Observatory
A. Pasqualetti - European Gravitational Observatory
R. Passaquieti - University of Pisa
D. Passuello - Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
M. Pedraza - California Institute of Technology
S. Penn - Hobart and William Smith Colleges
A. Perreca - Syracuse University
M. Phelps - California Institute of Technology
M. Pichot - Centre National de la Recherche Scientifique
M. Pickenpack - Max Planck Institute for Gravitational Physics
F. Piergiovanni - University of Urbino
V. Pierro - University of Sannio
L. Pinard - Centre National de la Recherche Scientifique
I.M. Pinto - University of Sannio
M. Pitkin - University of Glasgow
J. Poeld - Max Planck Institute for Gravitational Physics
R. Poggiani - University of Pisa
A. Poteomkin - Institute of Applied Physics
J. Powell - University of Glasgow
J. Prasad - Inter-University Centre for Astronomy and Astrophysics
S. Premachandra - Monash University
T. Prestegard - University of Minnesota
L.R. Price - California Institute of Technology
M. Prijatelj - European Gravitational Observatory
S. Privitera - California Institute of Technology
G.A. Prodi - University of Trento
L. Prokhorov - Lomonosov Moscow State University
O. Puncken - Brownsville Public Library
M. Punturo - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
P. Puppo - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
J. Qin - The University of Western Australia
V. Quetschke - Brownsville Public Library
E. Quintero - California Institute of Technology
G. Quiroga - Argentinian Gravitational Wave Group , Cordoba , Cordoba
R. Quitzow-James - University of Oregon
F.J. Raab - LIGO - Hanford Observatory
D.S. Rabeling - National Institute for Subatomic Physics
I. Rácz - HUN-REN Wigner Research Centre for Physics
H. Radkins - LIGO - Hanford Observatory
P. Raffai - Eötvös Loránd University
S. Raja - Raja Ramanna Centre for Advanced Technology
G. Rajalakshmi - Tata Institute of Fundamental Research
M. Rakhmanov - Brownsville Public Library
C. Ramet - LIGO Scientific Collaboration
K. Ramirez - Brownsville Public Library
P. Rapagnani - Sapienza University of Rome
V. Raymond - California Institute of Technology
V. Re - University of Rome Tor Vergata
J. Read - California State University, Fullerton
C.M. Reed - LIGO - Hanford Observatory
T. Regimbau - Centre National de la Recherche Scientifique
S. Reid - University of the West of Scotland
D.H. Reitze - California Institute of Technology
E. Rhoades - Embry–Riddle Aeronautical University
F. Ricci - Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
K. Riles - University of Michigan
N.A. Robertson - California Institute of Technology
F. Robinet - Université Paris-Sud
A. Rocchi - Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
M. Rodruck - LIGO - Hanford Observatory
L. Rolland - Centre National de la Recherche Scientifique
J.G. Rollins - California Institute of Technology
J.D. Romano - University of Texas at Brownsville
R. Romano - University of Salerno
G. Romanov - William & Mary
J.H. Romie - LIGO Scientific Collaboration
D. Rosińska - University of Zielona Góra
S. Rowan - University of Glasgow
A. Rüdiger - Max Planck Institute for Gravitational Physics
P. Ruggi - European Gravitational Observatory
K. Ryan - LIGO - Hanford Observatory
F. Salemi - Max Planck Institute for Gravitational Physics
L. Sammut - The University of Melbourne
V. Sandberg - LIGO - Hanford Observatory
J.R. Sanders - University of Michigan
V. Sannibale - California Institute of Technology
I. Santiago-Prieto - University of Glasgow
E. Saracco - Université Claude Bernard Lyon 1
B. Sassolas - Centre National de la Recherche Scientifique
B.S. Sathyaprakash - Cardiff University
P.R. Saulson - Syracuse University
R. Savage - LIGO - Hanford Observatory
J. Scheuer - Northwestern University
R. Schilling - Max Planck Institute for Gravitational Physics
R. Schnabel - Leibniz University Hannover
R.M.S. Schofield - University of Oregon
E. Schreiber - Max Planck Institute for Gravitational Physics
D. Schuette - Max Planck Institute for Gravitational Physics
B.F. Schutz - Max Planck Institute for Gravitational Physics
J. Scott - University of Glasgow
S.M. Scott - Australian National University
D. Sellers - LIGO Scientific Collaboration
A.S. Sengupta - Indian Institute of Technology Gandhinagar
D. Sentenac - European Gravitational Observatory
V. Sequino - University of Rome Tor Vergata
A. Sergeev - Institute of Applied Physics
D. Shaddock - Australian National University
S. Shah - Radboud University Nijmegen
M.S. Shahriar - Northwestern University
M. Shaltev - Max Planck Institute for Gravitational Physics
B. Shapiro - Stanford University
P. Shawhan - University of Maryland, College Park
D.H. Shoemaker - Massachusetts Institute of Technology
T.L. Sidery - University of Birmingham
K. Siellez - Centre National de la Recherche Scientifique
X. Siemens - University of Wisconsin–Milwaukee
D. Sigg - LIGO - Hanford Observatory
D. Simakov - Max Planck Institute for Gravitational Physics
A. Singer - California Institute of Technology
L. Singer - California Institute of Technology
R. Singh - Louisiana State University
A.M. Sintes - Universitat de les Illes Balears
B.J.J. Slagmolen - Australian National University
J. Slutsky - Max Planck Institute for Gravitational Physics
J.R. Smith - California State University, Fullerton
M. Smith - California Institute of Technology
R.J.E. Smith - California Institute of Technology
N.D. Smith-Lefebvre - California Institute of Technology
E.J. Son - National Institute for Mathematical Sciences
B. Sorazu - University of Glasgow
T. Souradeep - Inter-University Centre for Astronomy and Astrophysics
L. Sperandio - University of Rome Tor Vergata
A. Staley - Columbia University
J. Stebbins - Stanford University
J. Steinlechner - Max Planck Institute for Gravitational Physics
S. Steinlechner - Max Planck Institute for Gravitational Physics
B.C. Stephens - University of Wisconsin–Milwaukee
S. Steplewski - Washington State University
S. Stevenson - University of Birmingham
R. Stone - Brownsville Public Library
D. Stops - University of Birmingham
K.A. Strain - University of Glasgow
N. Straniero - Centre National de la Recherche Scientifique
S. Strigin - Lomonosov Moscow State University
R. Sturani - University of Urbino
A.L. Stuver - LIGO Scientific Collaboration
T.Z. Summerscales - Andrews University
S. Susmithan - The University of Western Australia
P.J. Sutton - Cardiff University
B. Swinkels - European Gravitational Observatory
M. Tacca - Université Paris Cité
D. Talukder - University of Oregon
D.B. Tanner - University of Florida
S.P. Tarabrin - Max Planck Institute for Gravitational Physics
R. Taylor - California Institute of Technology
A.P.M. Ter Braack - National Institute for Subatomic Physics
M.P. Thirugnanasambandam - California Institute of Technology
M. Thomas - LIGO Scientific Collaboration
P. Thomas - LIGO - Hanford Observatory
K.A. Thorne - LIGO Scientific Collaboration
K.S. Thorne - California Institute of Technology
E. Thrane - California Institute of Technology
V. Tiwari - University of Florida
K.V. Tokmakov - University of Strathclyde
C. Tomlinson - University of Sheffield
A. Toncelli - University of Pisa
M. Tonelli - University of Pisa
O. Torre - University of Siena
C.V. Torres - Brownsville Public Library
C.I. Torrie - California Institute of Technology
F. Travasso - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
G. Traylor - LIGO Scientific Collaboration
M. Tse - Massachusetts Institute of Technology
D. Ugolini - Trinity University
C.S. Unnikrishnan - Tata Institute of Fundamental Research
A.L. Urban - University of Wisconsin–Milwaukee
K. Urbanek - Stanford University
H. Vahlbruch - Leibniz University Hannover
G. Vajente - University of Pisa
G. Valdes - Brownsville Public Library
M. Vallisneri - California Institute of Technology
J.F.J. Van Den Brand - National Institute for Subatomic Physics
C. Van Den Broeck - National Institute for Subatomic Physics
S. Van Der Putten - National Institute for Subatomic Physics
M.V. Van Der Sluys - Radboud University Nijmegen
J. Van Heijningen - National Institute for Subatomic Physics
A.A. Van Veggel - University of Glasgow
S. Vass - California Institute of Technology
M. Vasúth - HUN-REN Wigner Research Centre for Physics
R. Vaulin - Massachusetts Institute of Technology
A. Vecchio - University of Birmingham
G. Vedovato - National Institute for Subatomic Physics
J. Veitch - University of Washington
P.J. Veitch - The University of Adelaide
K. Venkateswara - Centre National de la Recherche Scientifique
D. Verkindt - Centre National de la Recherche Scientifique
S.S. Verma - The University of Western Australia
F. Vetrano - University of Urbino
A. Viceré - Southern University and Agricultural and Mechanical College
R. Vincent-Finley - Southern University and Agricultural and Mechanical College
J.-Y. Vinet - Observatoire de la Côte d’Azur
S. Vitale - Massachusetts Institute of Technology
T. Vo - University of Perugia
H. Vocca - Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
C. Vorvick - University of Birmingham
W.D. Vousden - Lomonosov Moscow State University
S.P. Vyachanin - Lomonosov Moscow State University
A. Wade - University of Wisconsin–Milwaukee
L. Wade - University of Wisconsin–Milwaukee
M. Wade - Louisiana State University
M. Walker - Louisiana State University
L. Wallace - University of Birmingham
M. Wang - University of Birmingham
X. Wang - Australian National University
R.L. Ward - Australian National University
M. Was - Max Planck Institute for Gravitational Physics
B. Weaver - Centre National de la Recherche Scientifique
L.-W. Wei - Observatoire de la Côte d’Azur
M. Weinert - Max Planck Institute for Gravitational Physics
A.J. Weinstein - Massachusetts Institute of Technology
R. Weiss - LIGO Scientific Collaboration
T. Welborn - LIGO Scientific Collaboration
L. Wen - Max Planck Institute for Gravitational Physics
P. Wessels - Max Planck Institute for Gravitational Physics
M. West - Syracuse University
T. Westphal - Max Planck Institute for Gravitational Physics
K. Wette - Rochester Institute of Technology
J.T. Whelan - Rochester Institute of Technology
D.J. White - University of Sheffield
B.F. Whiting - University of Florida
K. Wiesner - Max Planck Institute for Gravitational Physics
C. Wilkinson - Southern University and Agricultural and Mechanical College
K. Williams - Southern University and Agricultural and Mechanical College
L. Williams - University of Florida
R. Williams - California Institute of Technology
T. Williams - Southeastern Louisiana University
A.R. Williamson - Cardiff University
J.L. Willis - Abilene Christian University
B. Willke - Leibniz University Hannover
M. Wimmer - Max Planck Institute for Gravitational Physics
W. Winkler - Massachusetts Institute of Technology
C.C. Wipf - University of Wisconsin–Milwaukee
A.G. Wiseman - University of Wisconsin–Milwaukee
H. Wittel - University of Glasgow
G. Woan - University of Glasgow
J. Worden - Northwestern University
J. Yablon - Northwestern University
I. Yakushin - LIGO Scientific Collaboration
H. Yamamoto - California Institute of Technology
C.C. Yancey - California Institute of Technology
H. Yang - California Institute of Technology
Z. Yang - Tsinghua University
S. Yoshida - Centre National de la Recherche Scientifique
M. Yvert - Centre National de la Recherche Scientifique
A. Zadrożny - Embry–Riddle Aeronautical University
M. Zanolin - Embry–Riddle Aeronautical University
J.-P. Zendri - Istituto Nazionale di Fisica Nucleare, Sezione di Padova
Fan Zhang - California Institute of Technology
L. Zhang - California Institute of Technology
C. Zhao - The University of Western Australia
X.J. Zhu - The University of Western Australia
M.E. Zucker - University of Massachusetts Amherst
S. Zuraw - University of Massachusetts Amherst
J. Zweizig - California Institute of Technology
Identifiers: 9957788165006774
Academic Unit: College of Electrical Engineering and Computer Science
Language: English
Resource Type: Journal article
Publication Details: Physical Review Letters, Vol.113(23), 231101

Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data

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