Comparison of half-mission temperature power spectra. The top panel shows the half-sum (HMHS; solid lines) and half-difference (HMHD; dashed lines) power spectra, while the bottom panel shows the difference between the half-sum and the best-fit Planck 2018 ΛCDM and half-difference spectra. The latter residual spectrum is binned with Δℓ = 25.
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