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Figure 21
Figure 21: Characteristic all-sky strain sensitivity for a burst wave having a bandwidth comparable to center frequency for the Cassini 2001 – 2002 data set [19]. This is the crudest measure of sky-averaged burst sensitivity: the square root of the product of the Doppler spectrum and the Fourier frequency, divided by the sky-averaged GW response (see Section 6.4).

J. W. Armstrong, "Low-Frequency Gravitational Wave Searches
Using Spacecraft Doppler Tracking",
Living Rev. Relativity, 9 (2006), 1, doi:10.12942/lrr-2006-1, URL (accessed <date>): http://www.livingreviews.org/lrr-2006-1.
© The author(s), except where otherwise noted. This work is licensed under a Creative Commons Attribution 4.0 International License.