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Fig. 9.
Ratio of the CIB × tSZ power spectra at different frequencies and at 217 × 217 GHz. The red curve shows the ratio with the CIB × tSZ template from Addison et al. (2012) used in the Planck Collaboration V (2020) likelihood analysis. All the power spectra are normalised such that they have the same value at ℓ = 3000.
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