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author = "Aasi, J. and Abadie, J. and Abbott, B. P. and Abbott, R. and
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Ast, S. and Aston, S. M. and Astone, P. and Aufmuth, P. and
Aulbert, C. and Austin, L. and Aylott, B. E. and Babak, S. and
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C. and Barker, D. and Barnum, S. H. and Barone, F. and Barr, B.
and Barsotti, L. and Barsuglia, M. and Barton, M. A. and Bartos,
I. and Bassiri, R. and Basti, A. and Batch, J. and Bauchrowitz, J.
and Bauer, Th. S. and Bebronne, M. and Behnke, B. and Bejger, M.
and Beker, M. G. and Bell, A. S. and Bell, C. and Belopolski, I.
and Bergmann, G. and Berliner, J. M. and Bertolini, A. and Bessis,
D. and Betzwieser, J. and Beyersdorf, P. T. and Bhadbhade, T. and
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and Bizouard, M. A. and Black, E. and Blackburn, J. K. and
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Bonelli, L. and Bonnand, R. and Bork, R. and Born, M. and Bose, S.
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and Braginsky, V. B. and Branchesi, M. and Brannen, C. A. and
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Zweizig, J. and Collaboration, LIGO Sci and Collaboration, Virgo",
affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {}
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and {} and {} and {} and {Instituto Nacional de Pesquisas
Espaciais (INPE)}",
title = "Directed search for continuous gravitational waves from the
Galactic center",
journal = "Physical Review D",
year = "2013",
volume = "88",
number = "10",
month = "Nov.",
keywords = "gravitational waves, galactic center, LIGO.",
abstract = "We present the results of a directed search for continuous
gravitational waves from unknown, isolated neutron stars in the
Galactic center region, performed on two years of data from LIGO's
fifth science run from two LIGO detectors. The search uses a
semicoherent approach, analyzing coherently 630 segments, each
spanning 11.5 hours, and then incoherently combining the results
of the single segments. It covers gravitational wave frequencies
in a range from 78 to 496 Hz and a frequency-dependent range of
first-order spindown values down to -7.86 x 10(-8) Hz/s at the
highest frequency. No gravitational waves were detected. The
90\\% confidence upper limits on the gravitational wave
amplitude of sources at the Galactic center are similar to 3.35 x
10(-25) for frequencies near 150 Hz. These upper limits are the
most constraining to date for a large-parameter-space search for
continuous gravitational wave signals.",
doi = "10.1103/PhysRevD.88.102002",
url = "http://dx.doi.org/10.1103/PhysRevD.88.102002",
issn = "1550-2368 and 1550-7998",
label = "isi 2014-01",
targetfile = "PhysRevD.88.102002.pdf",
urlaccessdate = "27 abr. 2024"
}