activity
19992019
most citedPlanck 2013 results. XXII. Constraints on inflation

1.1k citations · 9.4k across the 63 of their papers we have counts for

collaborators

63 papers

astro-ph.CO2019★ 495 cited

Planck 2018 results. VII. Isotropy and Statistics of the CMB

Planck Collaboration, Y. Akrami, M. Ashdown +147

Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in excellent agreement with pre…

astro-ph.CO2018★ 380 cited

Planck 2018 results. III. High Frequency Instrument data processing and frequency maps

Planck Collaboration, N. Aghanim, Y. Akrami +152

This paper presents the High Frequency Instrument (HFI) data processing procedures for the Planck 2018 release. Major improvements in mapmaking have been achieved since the previou…

astro-ph.CO2018★ 217 cited

Planck 2018 results. VI. Cosmological parameters

Planck Collaboration, N. Aghanim, Y. Akrami +179

We present cosmological parameter results from the final full-mission Planck measurements of the CMB anisotropies. We find good consistency with the standard spatially-flat 6-param…

astro-ph.CO2018★ 424 cited

Planck 2018 results. IV. Diffuse component separation

Planck Collaboration, Y. Akrami, M. Ashdown +150

We present full-sky maps of the cosmic microwave background (CMB) and polarized synchrotron and thermal dust emission, derived from the third set of Planck frequency maps. These pr…

astro-ph.CO2018★ 99 cited

Planck 2018 results. II. Low Frequency Instrument data processing

Planck Collaboration, Y. Akrami, F. Argüeso +148

We present a final description of the data-processing pipeline for the Planck, Low Frequency Instrument (LFI), implemented for the 2018 data release. Several improvements have been…

astro-ph.GA2018★ 203 cited

Planck 2018 results. XI. Polarized dust foregrounds

Planck Collaboration, Y. Akrami, M. Ashdown +131

The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic du…