@Article{LenziMaMaCoArAg:2008:SoInPr,
               author = "Lenzi, C{\'e}sar H. and Magalh{\~a}es, Nadja S. and Marinho Jr., 
                         Rubens M. and Costa, C{\'e}sar Augusto and Ara{\'u}jo, Helmo A. 
                         B. and Aguiar, Odylio Denys",
          affiliation = "{Instituto T{\'e}cnico Aeron{\'a}utico (ITA)} and {Centro 
                         Federal de Educa{\c{c}}{\~a}o de Tecnol{\'o}gica de S{\~a}o 
                         Paulo} and {Instituto T{\'e}cnico Aeron{\'a}utico (ITA)} and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto 
                         T{\'e}cnico Aeron{\'a}utico (ITA)} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)}",
                title = "Solution of the inverse problem in spherical gravitational wave 
                         detectors using a model with independent bars",
              journal = "Physical Review D",
                 year = "2008",
               volume = "78",
               number = "6",
                pages = "1--7",
                month = "Sept.",
                 note = "Erratum: C{\'e}sar H. Lenzi, Nadja S. Magalh{\~a}es, Rubens M. 
                         Marinho, C{\'e}sar A. Costa, Helmo A. Ara{\'u}jo, and Odylio D. 
                         Aguiar, Erratum: Solution of the inverse problem in spherical 
                         gravitational wave detectors using a model with independent bars 
                         [Phys. Rev. D 78, 062005 (2008)], Phys. Rev. D 78, 129901 
                         (2008).",
             keywords = "inverse problem, gravitational wave detectors, celestial 
                         objects.",
             abstract = "The direct detection of gravitational waves will provide valuable 
                         astrophysical information about many celestial objects. The 
                         SCHENBERG has already undergone its first test run. It is expected 
                         to have its first scientific run soon. In this work a new data 
                         analysis approach is presented, called the method of independent 
                         bars, which can be used with SCHENBERG's data. We test this method 
                         through the simulation of the detection of gravitational waves. 
                         With this method we find the source's direction without the need 
                         to have all six transducers operational. Also, we show that the 
                         method is a generalization of another one, already described in 
                         the literature, known as the mode channels method.",
                  doi = "10.1103/PhysRevD.78.062005",
                  url = "http://dx.doi.org/10.1103/PhysRevD.78.062005",
                 issn = "1550-2368 and 1550-7998",
             language = "en",
           targetfile = "PhysRevD.78.062005.pdf",
        urlaccessdate = "27 abr. 2024"
}