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Fig. 1.

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Characteristic strain as a function of frequency for 100 different realisations of a GWB with nominal amplitude 2.4 × 10−15. Each orange line corresponds to a different realisation (SMBHB population). The solid black line is the mean of those realisations, while the dashed black line highlights the nominal f−2/3 spectrum. The sensitivity curve is derived in The International Pulsar Timing Array Collaboration et al. (2023).

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