Fig. 11.
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Posterior distribution of the gravitational wave frequency fgw of a CGW fitted to two simulated PTAs: one with a single injected CGW (PSRN+CGW blue histogram), and one with an injected GWB (PSRN+GWB orange histogram). The posterior distribution is obtained with a MCMC analysis for a PSRN+CGW (Earth term) model. The dashed lines are the medians of the distributions.
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