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1
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85037219948
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For details of the LISA mission see http://lisa.jpl.nasa.gov
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For details of the LISA mission see http://lisa.jpl.nasa.gov
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9
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C. DeWitt, B. S. DeWitt
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Section 10.7 of Ya. B. Zel’dovich and I. D. Novikov, Relativistic Astrophysics, Vol. I, Stars and Relativity (U. Chicago Press, Chicago, 1971);also available as a Dover Reprint Volume.
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LISA Mission Definition Team and LISA Science Study Team, LISA: Laser Interferometer Space Antenna (March Press, Boulder, CO, 1999). The spectral density (Formula presented), as we have defined it, is related to the noise curve (Formula presented) shown in the figure on page 6 by (Formula presented) [P. Bender (private communication)]. Here (Formula presented) is the number of seconds in a year, and (Formula presented) where the (Formula presented) comes from averaging the noise over the sky and the 5 from the fact that the figure in this document is for a signal to noise ratio of 5
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LISA Mission Definition Team and LISA Science Study Team, LISA: Laser Interferometer Space Antenna (March Press, Boulder, CO, 1999). The spectral density (Formula presented), as we have defined it, is related to the noise curve (Formula presented) shown in the figure on page 6 by (Formula presented) [P. Bender (private communication)]. Here (Formula presented) is the number of seconds in a year, and (Formula presented) where the (Formula presented) comes from averaging the noise over the sky and the 5 from the fact that the figure in this document is for a signal to noise ratio of 5.
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18
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Mino, Y.1
Sasaki, M.2
Shibata, M.3
Tagoshi, H.4
Tanaka, T.5
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