Fig. 3.

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Maximum and standard deviation of temperature fluctuations for CMB photons that passed through a (100 Mpc)3 cosmological box. The box is populated with 109 M⊙ mergers according to a given volumetric merger rate, which are otherwise sampled uniformly in space, time, inclination, and orientation. The results are averaged over a total of ∼3 × 104 realisations (pale lines), an both the mean (solid lines) and the standard deviation (shaded areas enclosed by black lines) of the realisations are shown.
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