Fig. 5.
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As in Fig. 4, but for 100 h of SKA noise, where the noise is the dominant source of variance. We see now that WSTm is the statistic with the worst performance, and that WSTw, with its evolution along the lightcone summarised by the ℓ1-norm and ℓ2-norm on scales jz = 1, 2, which utilises wavelets derived from the power spectra binning, provides the tightest contours.
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