학술논문
BeyondPlanck XII. Cosmological parameter constraints with end-to-end error propagation
Document Type
Working Paper
Author
Paradiso, S.; Colombo, L. P. L.; Andersen, K. J.; Aurlien, R.; Banerji, R.; Basyrov, A.; Bersanelli, M.; Bertocco, S.; Brilenkov, M.; Carbone, M.; Eriksen, H. K.; Eskilt, J. R.; 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.; Partridge, B.; Reinecke, M.; San, M.; Suur-Uski, A. -S.; Svalheim, T. L.; Tavagnacco, D.; Thommesen, H.; Watts, D. J.; Wehus, I. K.; Zacchei, A.
Source
A&A 675, A12 (2023)
Subject
Language
Abstract
We present cosmological parameter constraints as estimated using the Bayesian BeyondPlanck (BP) analysis framework. This method supports seamless end-to-end error propagation from raw time-ordered data to final cosmological parameters. As a first demonstration of the method, we analyze time-ordered Planck LFI observations, combined with selected external data (WMAP 33-61GHz, Planck HFI DR4 353 and 857GHz, and Haslam 408MHz) in the form of pixelized maps which are used to break critical astrophysical degeneracies. Overall, all results are generally in good agreement with previously reported values from Planck 2018 and WMAP, with the largest relative difference for any parameter of about 1 sigma when considering only temperature multipoles between 29