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Svalheim, T. L.; Zonca, A.; Andersen, K. J.; Aurlien, R.; Banerji, R.; Bersanelli, M.; Bertocco, S.; Brilenkov, M.; Carbone, M.; Colombo, L. P. L.; Eriksen, H. K.; Foss, M. K.; Franceschet, C.; Fuskeland, U.; Galeotta, S.; Galloway, M.; Gerakakis, S.; Gjerløw, E.; Hensley, B.; Herman, D.; Iacobellis, M.; Ieronymaki, M.; Ihle, H. T.; Jewell, J. B.; Karakci, A.; Keihänen, E.; Keskitalo, R.; Maggio, G.; Maino, D.; Maris, M.; Paradiso, S.; Partridge, B.; Reinecke, M.; Suur-Uski, A. -S.; Tavagnacco, D.; Thommesen, H.; Watts, D. J.; Wehus, I. K.; Zacchei, A.
Astronomy and astrophysics (Berlin), 06/2023, Letnik: 675Journal Article
We discuss the treatment of bandpass and beam leakage corrections in the Bayesian BeyondPlanck CMB analysis pipeline as applied to the Planck LFI measurements. As a preparatory step, we first apply three corrections to the nominal LFI bandpass profiles including removal of a known systematic effect in the ground measuring equipment at 61 GHz; smoothing of standing wave ripples; and edge regularization. The main net impact of these modifications is an overall shift in the 70 GHz bandpass of +0.6 GHz; we argue that any analysis of LFI data products, either from Planck or BeyondPlanck, should use these new bandpasses. In addition, we fit a single free bandpass parameter for each radiometer of the form Δi = Δ0 + $δ$i , where Δ0 represents an absolute frequency shift per frequency band and $δ$i is a relative shift per detector. The absolute correction is only fitted at 30 GHz with a full $\chi$2 -based likelihood, resulting in a correction of Δ30 = 0.24 ± 0.03 GHz. The relative corrections are fitted using a spurious map approach, fundamentally similar to the method pioneered by the WMAP team, but without introducing many additional degrees of freedom. All bandpass parameters are sampled using a standard Metropolis sampler within the main BeyondPlanck Gibbs chain, and bandpass uncertainties are thus propagated to all other data products in the analysis. In total, we find that our bandpass model significantly reduces leakage effects. For beam leakage corrections, we adopt the official Planck LFI beam estimates without additional degrees of freedom, and only marginalize over the underlying sky model. We note that this is the first-time leakage from beam mismatch has been included for Planck LFI maps.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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