%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%@archivingpolicy denypublisher denyfinaldraft12
%@issn 0264-9381
%@resumeid
%@resumeid 8JMKD3MGP5W/3C9JJ2A
%@usergroup administrator
%@usergroup marciana
%@usergroup valdirene
%3 Response of the Brazilian gravitational wave detector.pdf
%X It is assumed that a black hole can be disturbed in such a way that a ringdown gravitational wave would be generated. This ringdown waveform is well understood and is modelled as an exponentially damped sinusoid. In this work, we use this kind of waveform to study the performance of the SCHENBERG gravitationalwave detector. This first realistic simulationwill help us to develop strategies for the signal analysis of this Brazilian detector. We calculated the signal-to-noise ratio as a function of frequency for the simulated signals and obtained results that  show that SCHENBERG is expected to be sensitive enough to detect this kind of signal up to a distance of ~20 kpc.
%8 Mar.
%N 5 Sp. Iss.
%@secondarydate 20040210
%T Response of the Brazilian gravitational wave detector to signals from a black hole ringdown
%@secondarytype PRE PI
%K mass, antenna, coalescences, sensitivity, merger, gravitational wave, schemberg model, black hole.
%@visibility shown
%@group DAS-INPE-MCT-BR
%@e-mailaddress cesar@das.inpe.br
%@secondarykey INPE-10781-PRE/6238
%@copyholder SID/SCD
%2 sid.inpe.br/jeferson/2004/06.30.15.53.50
%@affiliation Instituto Nacional de Pesquisas Espaciais - Divisão de Astrofísica
%@affiliation Instituto Tecnológico de Aeronáutica - Departamento de Física
%B Classical and Quantum Gravity
%P S827-S832
%4 sid.inpe.br/jeferson/2004/06.30.15.53
%D 2004
%V 21
%A Costa, César Augusto,
%A Aguiar, Odylio Denys de,
%A Magalhães, Nadja Simão,
%@dissemination WEBSCI; PORTALCAPES; COMPENDEX.
%@ 0264-9381
%@area CEA