author = "Aasi, J. and Abbott, B. P. and Abbott, R. and Abbott, T. and 
                         Abernathy, M. R. and Accadia, T. and Acernese, F. and Ackley, K. 
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                         and Affeldt, C. and Agathos, M. and Aggarwal, N. and Aguiar, 
                         Odylio Denys de and Ain, A. and Ajith, P. and Alemic, A. and 
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                         Bloemen, S. and Blom, M. and Bock, O. and Bodiya, T. P. and Boer, 
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                         T. and Bridges, D. O. and Brillet, A. and Brinkmann, M. and 
                         Brisson, V. and Brooks, A. F. and Brown, D. A. and Brown, D. D. 
                         and Br{\"u}ckner, F. and Buchman, S. and Bulik, T. and Bulten, H. 
                         J. and Buonanno, A. and Burman, R. and Buskulic, D. and Buy, C. 
                         and Cadonati, L. and Cagnoli, G. and Calder{\'o}n Bustillo, J. 
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                         Zweizig, J.",
          affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
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                         de Pesquisas Espaciais (INPE)}",
                title = "Search for gravitational radiation from intermediate mass black 
                         hole binaries in data from the second LIGO-Virgo joint science 
              journal = "Physical Review D",
                 year = "2014",
               volume = "89",
               number = "12",
                pages = "122003 (15pp.)",
             abstract = "This paper reports on an unmodeled, all-sky search for 
                         gravitational waves from merging intermediate mass black hole 
                         binaries (IMBHB). The search was performed on data from the second 
                         joint science run of the LIGO and Virgo detectors (July 
                         2009-October 2010) and was sensitive to IMBHBs with a range up to 
                         <200Mpc, averaged over the possible sky positions and inclinations 
                         of the binaries with respect to the line of sight. No significant 
                         candidate was found. Upper limits on the coalescence-rate density 
                         of nonspinning IMBHBs with total masses between 100 and 450M and 
                         mass ratios between 0.25 and 1 were placed by combining this 
                         analysis with an analogous search performed on data from the first 
                         LIGO-Virgo joint science run (November 2005-October 2007). The 
                         most stringent limit was set for systems consisting of two 88M 
                         black holes and is equal to 0.12Mpc-3Myr-1 at the 90% confidence 
                         level. This paper also presents the first estimate, for the case 
                         of an unmodeled analysis, of the impact on the search range of 
                         IMBHB spin configurations: the visible volume for IMBHBs with 
                         nonspinning components is roughly doubled for a population of 
                         IMBHBs with spins aligned with the binary's orbital angular 
                         momentum and uniformly distributed in the dimensionless spin 
                         parameter up to 0.8, whereas an analogous population with 
                         antialigned spins decreases the visible volume by ~20%.",
                  doi = "10.1103/PhysRevD.89.122003",
                  url = "http://dx.doi.org/10.1103/PhysRevD.89.122003",
                 issn = "1550-2368 and 1550-7998",
                label = "scopus 2014-07 
             language = "en",
           targetfile = "PhysRevD.89.122003.pdf",
        urlaccessdate = "16 jan. 2021"