Astrophysical: Cosmic background radiation

  • Publication
    Planck 2018 results. I. Overview and the cosmological legacy of Planck
    The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It...
  • Publication
    Planck 2018 results. II. Low Frequency Instrument data processing
    We present a final description of the data-processing pipeline for the Planck Low Frequency Instrument (LFI), implemented for the 2018 data release. Several...
  • Publication
    Planck 2018 results. III. High Frequency Instrument data processing and frequency maps
    This paper presents the High Frequency Instrument (HFI) data processing procedures for the Planck 2018 release. Major improvements in mapmaking have been...
  • Publication
    Planck 2018 results. IV. Diffuse component separation
    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...
  • Publication
    Planck 2018 results. IX. Constraints on primordial non-Gaussianity
    We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non...
  • Publication
    Planck 2018 results. V. CMB power spectra and likelihoods
    We describe the legacy Planck cosmic microwave background (CMB) likelihoods derived from the 2018 data release. The overall approach is similar in spirit to the...
  • Publication
    Planck 2018 results. VI. Cosmological parameters
    We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining...
  • Publication
    Planck 2018 results. VI. Cosmological parameters (Corrigendum)
  • Publication
    Planck 2018 results. VII. Isotropy and statistics of the CMB
    Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in...