Fig. C.1
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Top: Maximal chirp mass ℳ of a binary system for which the assumption of a constant GW frequency Pgw gives a maximal phase error of ϱ = 0.25, 0.5, and 1 rad over the duration of observations T = 5 yr (circular orbit assumed for the binary). Bottom: Maximal strain h under the same conditions, assuming a luminosity distance of r= 100 Mpc.
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