Planck intermediate results. LVII. Joint Planck LFI and HFI data 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 ($3366.6\pm 2.7$)$\mu$K, consistent with, albeit slightly higher than, earlier estimates. From the large-scale polarization data, we derive an updated estimate of the optical depth of reionization of $\tau =0.051\pm 0.006$, which appears robust with respect to data and sky cuts. There are 600 complete signal, noise and systematics simulations of the full-frequency and detector-set maps. As a Planck first, these simulations include full time-domain processing of the beam-convolved CMB anisotropies. The release of NPIPE maps and simulations is accompanied with a complete suite of raw and processed time-ordered data and the software, scripts, auxiliary data, and parameter files needed to improve further on the analysis and to run matching simulations.

97 pages, 93 figures and 16 tables, abstract abridged for arXiv submission, accepted for publication in A&A

References in corpus (66)

• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• The Milky Way in Molecular Clouds: A New Complete CO Survey
• Planck 2013 results. I. Overview of products and scientific results
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Planck 2018 results. I. Overview and the cosmological legacy of Planck
• The Temperature of the Cosmic Microwave Background
• Planck 2018 results. V. CMB power spectra and likelihoods
• The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: II. Model of the Interplanetary Dust Cloud
• Planck 2018 results. VII. Isotropy and Statistics of the CMB
• Planck 2018 results. IV. Diffuse component separation
• Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth
• Planck 2018 results. III. High Frequency Instrument data processing and frequency maps
• Joint Bayesian component separation and CMB power spectrum estimation
• Planck 2013 results. XII. Component separation
• Planck 2015 results. X. Diffuse component separation: Foreground maps
• Planck 2015 results. IX. Diffuse component separation: CMB maps
• Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps
• Component separation methods for the Planck mission
• Likelihood Analysis of CMB Temperature and Polarization Power Spectra
• Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
• Fast estimation of polarization power spectra using correlation functions
• Planck intermediate results. XLVII. Planck constraints on reionization history
• Global, Exact Cosmic Microwave Background Data Analysis Using Gibbs Sampling
• The Dipole Observed in the COBE DMR Four-Year Data
• Power spectrum estimation from high-resolution maps by Gibbs sampling
• Planck 2018 results. XI. Polarized dust foregrounds
• Planck 2013 results. IX. HFI spectral response
• Planck 2015 results. XXI. The integrated Sachs-Wolfe effect
• How to measure CMB polarization power spectra without losing information
• Foreground component separation with generalised ILC
• Planck early results. VI. The High Frequency Instrument data processing
• Xspect, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars
• A new, large-scale map of interstellar reddening derived from HI emission
• Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources
• Planck 2013 results. VI. High Frequency Instrument data processing
• Application of Monte Carlo Algorithms to the Bayesian Analysis of the Cosmic Microwave Background
• Planck 2013 results. XIV. Zodiacal emission
• Planck pre-launch status: High Frequency Instrument polarization calibration
• Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds
• Planck 2018 results. II. Low Frequency Instrument data processing
• Multi-resolution internal template cleaning: An application to the Wilkinson Microwave Anisotropy Probe 7-yr polarization data
• Planck 2013 results. II. Low Frequency Instrument data processing
• Planck 2015 results. V. LFI calibration
• Planck 2013 results X. Energetic particle effects: characterization, removal, and simulation
• Libsharp - spherical harmonic transforms revisited
• Planck 2015 results. XII. Full Focal Plane simulations
• Planck 2013 results. V. LFI calibration
• Comparison of filters for the detection of point sources in Planck simulations
• Planck 2015 results. VII. HFI TOI and beam processing
• SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps
• Planck 2015 results. II. Low Frequency Instrument data processing
• Madam - a map-making method for CMB experiments
• Making CMB temperature and polarization maps with Madam
• A maximum likelihood approach to the destriping technique
• Large-scale CMB temperature and polarization cross-spectra likelihoods
• Destriping CMB temperature and polarization maps
• The geometry of the magnetic field in the Central Molecular Zone measured by PILOT
• QuickPol: Fast calculation of effective beam matrices for CMB polarization
• On the proper kinetic quadrupole CMB removal and the quadrupole anomalies
• Algorithm for the evaluation of reduced Wigner matrices
• Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations
• Quadratic estimator for CMB cross-correlation
• Multi-resolution Bayesian CMB component separation through Wiener-filtering with a pseudo-inverse preconditioner
• Detection/estimation of the modulus of a vector. Application to point source detection in polarization data
• Planck pre-launch status: calibration of the Low Frequency Instrument flight model radiometers

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