Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
Planck Collaboration: Y. Akrami, K. J. Andersen, M. Ashdown, C., Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, S., Basak, K. Benabed, J.-P. Bernard, M. Bersanelli, P. Bielewicz, J. R. Bond, J., Borrill, C. Burigana, R. C. Butler, E. Calabrese

TL;DR
The paper introduces the NPIPE processing pipeline for Planck data, significantly reducing noise and systematics, and provides new measurements of the Solar dipole and reionization optical depth using combined LFI and HFI data.
Contribution
It presents a new data processing pipeline that improves calibration, reduces noise, and enhances consistency in Planck frequency maps, enabling more precise cosmological measurements.
Findings
First estimate of the Solar dipole amplitude from combined frequencies.
Updated optical depth of reionization: τ = 0.051 ± 0.006.
Comprehensive simulations including full time-domain processing.
Abstract
We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High Frequency Instrument (HFI) using high-performance computers. NPIPE represents a natural evolution of previous Planck analysis efforts, and combines some of the most powerful features of the separate LFI and HFI analysis pipelines. The net effect of the improvements is lower levels of noise and systematics in both frequency and component maps at essentially all angular scales, as well as notably improved internal consistency between the various frequency channels. Based on the NPIPE maps, we present the first estimate of the Solar dipole determined through component separation across all nine Planck frequencies. The amplitude is ()K, consistent with, albeit slightly higher than, earlier…
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