This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz,
which is the most sensitive Planck channel for dust polarization. We construct and analyse …

This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz,
which is the most sensitive Planck channel for dust polarization. We construct and analyse …

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 …

The European Space Agency's Planck satellite, dedicated to studying the early Universe
and its subsequent evolution, was launched 14 May 2009 and has been scanning the …

We analyse the implications of the Planck data for cosmic inflation. The Planck nominal
mission temperature anisotropy measurements, combined with the WMAP large-angle …

We present constraints on cosmological parameters using number counts as a function of
redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The …

This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857
GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky …

This paper presents cosmological results based on full-mission Planck observations of
temperature and polarization anisotropies of the cosmic microwave background (CMB) …

We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results …

The two fundamental assumptions of the standard cosmological model–that the initial
fluctuations are statistically isotropic and Gaussian–are rigorously tested using maps of the …