@Article{CostaAguiMaga:2004:ReBrGr,
author = "Costa, C{\'e}sar Augusto and Aguiar, Odylio Denys de and
Magalh{\~a}es, Nadja Sim{\~a}o",
affiliation = "{Instituto Nacional de Pesquisas Espaciais - Divis{\~a}o de
Astrof{\'{\i}}sica} and {Instituto Tecnol{\'o}gico de
Aeron{\'a}utica - Departamento de F{\'{\i}}sica}",
title = "Response of the Brazilian gravitational wave detector to signals
from a black hole ringdown",
journal = "Classical and Quantum Gravity",
year = "2004",
volume = "21",
number = "5 Sp. Iss.",
pages = "S827--S832",
month = "Mar.",
keywords = "mass, antenna, coalescences, sensitivity, merger, gravitational
wave, schemberg model, black hole.",
abstract = "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.",
copyholder = "SID/SCD",
isbn/issn = "0264-9381",
issn = "0264-9381",
language = "en",
targetfile = "Response of the Brazilian gravitational wave detector.pdf",
urlaccessdate = "09 maio 2024"
}