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@article{Abbott:2009:10.1103/PhysRevD.80.102001,
author = {Abbott, BP and Abbott, R and Adhikari, R and Ajith, P and Allen, B and Allen, G and Amin, RS and Anderson, SB and Anderson, WG and Arain, MA and Araya, M and Armandula, H and Armor, P and Aso, Y and Aston, S and Aufmuth, P and Aulbert, C and Babak, S and Baker, P and Ballmer, S and Barker, C and Barker, D and Barr, B and Barriga, P and Barsotti, L and Barton, MA and Bartos, I and Bassiri, R and Bastarrika, M and Behnke, B and Benacquista, M and Betzwieser, J and Beyersdorf, PT and Bilenko, IA and Billingsley, G and Biswas, R and Black, E and Blackburn, JK and Blackburn, L and Blair, D and Bland, B and Bodiya, TP and Bogue, L and Bork, R and Boschi, V and Bose, S and Brady, PR and Braginsky, VB and Brau, JE and Bridges, DO and Brinkmann, M and Brooks, AF and Brown, DA and Brummit, A and Brunet, G and Bullington, A and Buonanno, A and Burmeister, O and Byer, RL and Cadonati, L and Camp, JB and Cannizzo, J and Cannon, KC and Cao, J and Cardenas, L and Caride, S and Castaldi, G and Caudill},
doi = {10.1103/PhysRevD.80.102001},
journal = {Physical Review D Particles Fields Gravitation and Cosmology},
title = {Search for gravitational-wave bursts in the first year of the fifth LIGO science run},
url = {http://dx.doi.org/10.1103/PhysRevD.80.102001},
volume = {80},
year = {2009}
}
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TY  - JOUR
AB  - We present the results obtained from an all-sky search for gravitational-wave (GW) bursts in the 64-2000 Hz frequency range in data collected by the LIGO detectors during the first year (November 2005-November 2006) of their fifth science run. The total analyzed live time was 268.6 days. Multiple hierarchical data analysis methods were invoked in this search. The overall sensitivity expressed in terms of the root-sum-square (rss) strain amplitude hrss for gravitational-wave bursts with various morphologies was in the range of 6×10-22Hz-1/2 to a few×10-21Hz-1/2. No GW signals were observed and a frequentist upper limit of 3.75 events per year on the rate of strong GW bursts was placed at the 90% confidence level. As in our previous searches, we also combined this rate limit with the detection efficiency for selected waveform morphologies to obtain event rate versus strength exclusion curves. In sensitivity, these exclusion curves are the most stringent to date. © 2009 The American Physical Society.
AU  - Abbott,BP
AU  - Abbott,R
AU  - Adhikari,R
AU  - Ajith,P
AU  - Allen,B
AU  - Allen,G
AU  - Amin,RS
AU  - Anderson,SB
AU  - Anderson,WG
AU  - Arain,MA
AU  - Araya,M
AU  - Armandula,H
AU  - Armor,P
AU  - Aso,Y
AU  - Aston,S
AU  - Aufmuth,P
AU  - Aulbert,C
AU  - Babak,S
AU  - Baker,P
AU  - Ballmer,S
AU  - Barker,C
AU  - Barker,D
AU  - Barr,B
AU  - Barriga,P
AU  - Barsotti,L
AU  - Barton,MA
AU  - Bartos,I
AU  - Bassiri,R
AU  - Bastarrika,M
AU  - Behnke,B
AU  - Benacquista,M
AU  - Betzwieser,J
AU  - Beyersdorf,PT
AU  - Bilenko,IA
AU  - Billingsley,G
AU  - Biswas,R
AU  - Black,E
AU  - Blackburn,JK
AU  - Blackburn,L
AU  - Blair,D
AU  - Bland,B
AU  - Bodiya,TP
AU  - Bogue,L
AU  - Bork,R
AU  - Boschi,V
AU  - Bose,S
AU  - Brady,PR
AU  - Braginsky,VB
AU  - Brau,JE
AU  - Bridges,DO
AU  - Brinkmann,M
AU  - Brooks,AF
AU  - Brown,DA
AU  - Brummit,A
AU  - Brunet,G
AU  - Bullington,A
AU  - Buonanno,A
AU  - Burmeister,O
AU  - Byer,RL
AU  - Cadonati,L
AU  - Camp,JB
AU  - Cannizzo,J
AU  - Cannon,KC
AU  - Cao,J
AU  - Cardenas,L
AU  - Caride,S
AU  - Castaldi,G
AU  - Caudill,S
AU  - Cavaglià,M
AU  - Cepeda,C
AU  - Chalermsongsak,T
AU  - Chalkley,E
AU  - Charlton,P
AU  - Chatterji,S
AU  - Chelkowski,S
AU  - Chen,Y
AU  - Christensen,N
AU  - Chung,CTY
AU  - Clark,D
AU  - Clark,J
AU  - Clayton,JH
AU  - Cokelaer,T
AU  - Colacino,CN
AU  - Conte,R
AU  - Cook,D
AU  - Corbitt,TRC
AU  - Cornish,N
AU  - Coward,D
AU  - Coyne,DC
AU  - Creighton,JDE
AU  - Creighton,TD
AU  - Cruise,AM
AU  - Culter,RM
AU  - Cumming,A
AU  - Cunningham,L
AU  - Danilishin,SL
AU  - Danzmann,K
AU  - Daudert,B
AU  - Davies,G
AU  - Daw,EJ
DO  - 10.1103/PhysRevD.80.102001
PY  - 2009///
SN  - 1550-7998
TI  - Search for gravitational-wave bursts in the first year of the fifth LIGO science run
T2  - Physical Review D Particles Fields Gravitation and Cosmology
UR  - http://dx.doi.org/10.1103/PhysRevD.80.102001
VL  - 80
ER  -
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