@InProceedings{MagalhãesPFMMOAJ:2009:SeMoSi,
author = "Magalh{\~a}es, Nadja S. and Pires, Ricardo and Frajuca, Carlos
and Melo, Rafael F. and Marinho J{\'u}nior, Rubens M. and
Oliveria, Fernanda G. and Aguiar, Odylio Denys and Johson, Warren
W.",
affiliation = "UNIFESP and IFSP and IFSP and IFSP and ITA and ITA and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and LSU",
title = "Searching for Monochromatic Signals in Gravitational Wave
Detection",
year = "2009",
organization = "Encontro Nacional de F{\'{\i}}sica de Part{\'{\i}}culas e
Campos, 30.",
abstract = "This work focus on the detection of continuous gravitational wave
signals. A new data analysis is proposed based on a method
tailored for the detection of monochromatic signals in the middle
of strong, white noise. Known in the literature as the Welch
method, it basically makes power spectrum estimates using averaged
modified periodograms. The averaging procedure reduces white
noise, which is random, while evidencing monochromatic signals.
Therefore, by using this method it is possible to obtain a power
spectrum for the data which preserves peaks due to monochromatic
signals. Then an analysis is performed on persistent peaks,
searching for frequency drifts that might present a pattern
similar to the one due to Doppler shifts. In gravitational wave
detection two kinds of Doppler shifts are expected, with annual
and daily periods. For the chosen data set of the ALLEGRO
gravitational wave detector it was found that none of the
strongest, persistent peaks investigated presented a frequency
drift with a Doppler shift pattern, thus excluding them as
gravitational wave signal candidates. The method proved useful
even for very noisy data, by minimizing the noise to levels much
inferior to the monochromatic signal ones and allowing the Doppler
shift analysis. It can be used with interferometric detectors as
well.",
conference-location = "Passa Quatro, MG",
conference-year = "14-18 set.",
urlaccessdate = "28 abr. 2024"
}