@Article{LenziMaCoMaArAg:2008:AsDaAn,
               author = "Lenzi, C{\'e}sar H. and Magalh{\~a}es, Nadja S. and Costa, 
                         C{\'e}sar Augusto and Marinho J{\'u}nior, Rubens M. and 
                         Ara{\'u}jo, Helmo A. B. and Aguiar, Odylio Denys de",
          affiliation = "Departamento de F{\'{\i}}sica, Instituto Tecnol{\'o}gico de 
                         Aeron{\'a}utica and {Centro Federal de Educa{\c{c}}{\~a}o 
                         Tecnol{\'o}gica de S{\~a}o Paulo} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and Departamento de F{\'{\i}}sica, 
                         Instituto Tecnol{\'o}gico de Aeron{\'a}utica and Departamento de 
                         F{\'{\i}}sica, Instituto Tecnol{\'o}gico de Aeron{\'a}utica 
                         and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Astrophysics from data analysis of spherical gravitational wave 
                         detectors",
              journal = "General Relativity and Gravitation",
                 year = "2008",
               volume = "40",
               number = "1",
                pages = "183--190",
                month = "Jan.",
             keywords = "Gravitational waves - Spherical gravitational wave detector - 
                         Inverse problem solution - Method of independent bars.",
             abstract = "The direct detection of gravitational waves will provide valuable 
                         astrophysical information about many celestial objects. Also, it 
                         will be an important test to general relativity and other theories 
                         of gravitation. The gravitational wave detector SCHENBERG has 
                         recently undergone its first test run. It is expected to have its 
                         first scientific run soon. In this work the data analysis system 
                         of this spherical, resonant mass detector is tested through the 
                         simulation of the detection of gravitational waves generated 
                         during the inspiralling phase of a binary system. It is shown from 
                         the simulated data that it is not necessary to have all six 
                         transducers operational in order to determine the sources 
                         direction and the waves amplitudes.",
           copyholder = "SID/SCD",
                  doi = "10.1007/s10714-007-0524-1",
                  url = "http://dx.doi.org/10.1007/s10714-007-0524-1",
                 issn = "0001-7701",
             language = "en",
           targetfile = "astrophysics from data.pdf",
        urlaccessdate = "27 abr. 2024"
}