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@Article{AbadieAAAAAAAAAAAAACAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCDDDDDDDDDDDDRDDDPDDDDDDDDEDDDDDDDDDDDEEEEEEEEEEEFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHIIIIIJJJJJJJJJJKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNNNNNNNNNNNOOOOOOOOOOOOOOPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPQQRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSTTTTTTTTTTTTTTTTTTTTTTTTUVVBVPVVVVVVVVVVVVVVVVVVVWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWYYYYYYYYYZZZZZZZZZZCC:2012:AlSeGr,
               author = "Abadie, J. and Abbott, B. P. and Abbott, R. and Abbott, T. D. and 
                         Abernathy, M. and Accadia, T. and Acernese, F. and Adams, C. and 
                         Adhikari, R. and Affeldt, C. and Agathos, M. and Agatsuma, K. and 
                         Ajith, P. and Allen, B. and Ceron, E. Amador and Amariutei, D. and 
                         Anderson, S. B. and Anderson, W. G. and Arai, K. and Arain, M. A. 
                         and Araya, M. C. and Aston, S. M. and Astone, P. and Atkinson, D. 
                         and Aufmuth, P. and Aulbert, C. and Aylott, B. E. and Babak, S. 
                         and Baker, P. and Ballardin, G. and Ballmer, S. and Barayoga, J. 
                         C. B. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L. 
                         and Barsuglia, M. and Barton, M. A. and Bartos, I. and Bassiri, R. 
                         and Bastarrika, M. and Basti, A. and Batch, J. and Bauchrowitz, J. 
                         and Bauer, Th. S. and Bebronne, M. and Beck, D. and Behnke, B. and 
                         Bejger, M. and Beker, M. G. and Bell, A. S. and Belletoile, A. and 
                         Belopolski, I. and Benacquista, M. and Berliner, J. M. and 
                         Bertolini, A. and Betzwieser, J. and Beveridge, N. and Beyersdorf, 
                         P. T. and Bilenko, I. A. and Billingsley, G. and Birch, J. and 
                         Biswas, R. and Bitossi, M. and Bizouard, M. A. and Black, E. and 
                         Blackburn, J. K. and Blackburn, L. and Blair, D. and Bland, B. and 
                         Blom, M. and Bock, O. and Bodiya, T. P. and Bogan, C. and 
                         Bondarescu, R. and Bondu, F. and Bonelli, L. and Bonnand, R. and 
                         Bork, R. and Born, M. and Boschi, V. and Bose, S. and Bosi, L. and 
                         Bouhou, B. and Braccini, S. and Bradaschia, C. and Brady, P. R. 
                         and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Breyer, 
                         J. and Briant, T. and Bridges, D. O. and Brillet, A. and 
                         Brinkmann, M. and Brisson, V. and Britzger, M. and Brooks, A. F. 
                         and Brown, D. A. and Bulik, T. and Bulten, H. J. and Buonanno, A. 
                         and Burguet-Castell, J. and Buskulic, D. and Buy, C. and Byer, R. 
                         L. and Cadonati, L. and Cagnoli, G. and Calloni, E. and Camp, J. 
                         B. and Campsie, P. and Cannizzo, J. and Cannon, K. and Canuel, B. 
                         and Cao, J. and Capano, C. D. and Carbognani, F. and Carbone, L. 
                         and Caride, S. and Caudill, S. and Cavaglia, M. and Cavalier, F. 
                         and Cavalieri, R. and Cella, G. and Cepeda, C. and Cesarini, E. 
                         and Chaibi, O. and Chalermsongsak, T. and Charlton, P. and 
                         Chassande-Mottin, E. and Chelkowski, S. and Chen, W. and Chen, X. 
                         and Chen, Y. and Chincarini, A. and Chiummo, A. and Cho, H. S. and 
                         Chow, J. and Christensen, N. and Chua, S. S. Y. and Chung, C. T. 
                         Y. and Chung, S. and Ciani, G. and Clara, F. and Clark, D. E. and 
                         Clark, J. and Clayton, J. H. and Cleva, F. and Coccia, E. and 
                         Cohadon, P. -F. and Colacino, C. N. and Colas, J. and Colla, A. 
                         and Colombini, M. and Conte, A. and Conte, R. and Cook, D. and 
                         Corbitt, T. R. and Cordier, M. and Cornish, N. and Corsi, A. and 
                         Costa, C{\'e}sar Augusto and Coughlin, M. and Coulon, J. -P. and 
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                         Collaboration, LIGO Sci and Collaboration, Virgo",
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                         {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "All-sky search for gravitational-wave bursts in the second joint 
                         LIGO-Virgo run",
              journal = "Physical Review D",
                 year = "2012",
               volume = "85",
               number = "12",
                pages = "122007--1_15",
                month = "Jun.",
             keywords = "gravitational-wave bursts, LIGO-Virgo detectors.",
             abstract = "We present results from a search for gravitational-wave bursts in 
                         the data collected by the LIGO and Virgo detectors between July 7, 
                         2009 and October 20, 2010: data are analyzed when at least two of 
                         the three LIGO-Virgo detectors are in coincident operation, with a 
                         total observation time of 207 days. The analysis searches for 
                         transients of duration less than or similar to 1 s over the 
                         frequency band 64-5000 Hz, without other assumptions on the signal 
                         waveform, polarization, direction or occurrence time. All 
                         identified events are consistent with the expected accidental 
                         background. We set frequentist upper limits on the rate of 
                         gravitational-wave bursts by combining this search with the 
                         previous LIGO-Virgo search on the data collected between November 
                         2005 and October 2007. The upper limit on the rate of strong 
                         gravitational-wave bursts at the Earth is 1.3 events per year at 
                         90\\% confidence. We also present upper limits on source rate 
                         density per year and Mpc(3) for sample populations of 
                         standard-candle sources. As in the previous joint run, typical 
                         sensitivities of the search in terms of the root-sum-squared 
                         strain amplitude for these waveforms lie in the range similar to 5 
                         x 10(-22) Hz(-1/2) to similar to 1 x 10(-20) Hz(-1/2). The 
                         combination of the two joint runs entails the most sensitive 
                         all-sky search for generic gravitational-wave bursts and 
                         synthesizes the results achieved by the initial generation of 
                         interferometric detectors.",
                  doi = "10.1103/PhysRevD.85.122007",
                  url = "http://dx.doi.org/10.1103/PhysRevD.85.122007",
                 issn = "1550-2368 and 1550-7998",
             language = "en",
           targetfile = "PhysRevD.85.122007.pdf",
        urlaccessdate = "24 jan. 2021"
}


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