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- bibnamefont
bibfnamefont
url
urlprefix
- 1
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B. Allen,
GRASP: a data analysis package for gravitational wave
detection, Department of Physics, P.O. Box 413,
University of Wisconsin, Milwaukee WI 53201, USA, 1st ed.
(2000), http:
www.lsc-group.phys.uwm.edu
ballengrasp-distribution.
- 2
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C. M. Will and
A. G. Wiseman,
Phys. Rev. D. 54(8), 4813 (1996).
- 3
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W. G. Anderson,
P. R. Brady,
J. D. E. Creighton,
and É. É.
Flanagan, An excess power statistic for
detection of burst sources of gravitational radiation
(2000), gr-qc/0008066.
- 4
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K. R. Lang,
Astrophysical Formulae, Volume II: Space, Time, Matter
and Cosmology, Astronomy and Astrophysics Library
(Springer-Verlag, Berlin,
1999), 3rd ed.
- 5
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B. Allen and J. D. Romano, ``Detecting a stochastic background of
gravitational radiation: Signal processing strategies and
sensitivities''
Phys. Rev. D 59, 102001 (1999);
http://www.arXiv.org/abs/gr-qc/9710117gr-qc/9710117
- 6
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E. Flanagan, ``The sensitivity of the laser interferometer gravitational
wave observatory (LIGO) to a stochastic background, and its dependence on
the detector orientations''
Phys. Rev. D 48, 2389 (1993);
http://www.arXiv.org/abs/astro-ph/9305029astro-ph/9305029
Subsections
LAL test account
2003-10-23