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Fig. 2.
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Detset cross-spectra for half-ring differences computed on 75% of the sky, divided by their uncertainties. From top to bottom we show: TT, EE, TE, and ET. Spectra are binned with Δℓ = 40. The projections on the right show the distribution for each unbinned spectrum over the range ℓ = 30–2500.
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