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                         H. J. and Buonanno, A. and Burman, R. and Buskulic, D. and Buy, C. 
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          affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
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                         {} and {} and {} and {} and {} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Search for gravitational wave ringdowns from perturbed 
                         intermediate mass black holes in LIGO-Virgo data from 2005-2010",
              journal = "Physical Review D",
                 year = "2014",
               volume = "89",
               number = "10",
                pages = "102006 (18pp.)",
             abstract = "We report results from a search for gravitational waves produced 
                         by perturbed intermediate mass black holes (IMBH) in data 
                         collected by LIGO and Virgo between 2005 and 2010. The search was 
                         sensitive to astrophysical sources that produced damped sinusoid 
                         gravitational wave signals, also known as ringdowns, with 
                         frequency 50df0/Hzd2000 and decay timescale 0.0001 {\"A}/s 0.1 
                         characteristic of those produced in mergers of IMBH pairs. No 
                         significant gravitational wave candidate was detected. We report 
                         upper limits on the astrophysical coalescence rates of IMBHs with 
                         total binary mass 50dM/M d450 and component mass ratios of either 
                         1:1 or 4:1. For systems with total mass 100dM/M d150, we report a 
                         90% confidence upper limit on the rate of binary IMBH mergers with 
                         nonspinning and equal mass components of 6.9×10-8Mpc-3yr-1. We 
                         also report a rate upper limit for ringdown waveforms from 
                         perturbed IMBHs, radiating 1% of their mass as gravitational waves 
                         in the fundamental, = m=2, oscillation mode, that is nearly three 
                         orders of magnitude more stringent than previous results. © 2014 
                         American Physical Society.",
                  doi = "10.1103/PhysRevD.89.102006",
                  url = "http://dx.doi.org/10.1103/PhysRevD.89.102006",
                 issn = "1550-2368 and 1550-7998",
                label = "scopus 2014-07 
             language = "en",
           targetfile = "PhysRevD.89.102006.pdf",
        urlaccessdate = "16 jan. 2021"