Fig. 17.
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Comparison of noise power spectra from BEYONDPLANCK (black), Planck 2018 (red) and PR4 (blue); We report the Planck 2018 best-fit with a dotted line, and the BEYONDPLANCK white noise contribution as a dashed line. Each dataset includes a regularization noise of 2 μK/pixel for temperature, and 0.02 μK/pixel for polarization.
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