… Finally, we apply SMICA-specific temperature and polarization masks described in Planck
Collaboration IX (2016). Combining all three sets of masks leaves a total of 67.3% of the sky …

… (Planck Collaboration Int. XLVI 2016), we derive the first estimate of τ from the Planck-HFI …
9). This confirms that there is only a modest amount of information in the angular shape of …

… of the nine Planck frequency maps and their characteristics. Section 8 describes the Planck
2015 … Section 9 describes the Planck 2015 astrophysical products, including catalogues of …

This paper presents the characterization of the in-flight beams, the beam window functions,
and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The …

… In March 2013, the Planck Consortium released its first temperature measurements of the …
in terms of nine frequency maps between 30 and 857 GHz (Planck Collaboration I 2014). The …

… using the Planck likelihood, which is described in detail in Planck Collaboration XI (2016). …
The Planck likelihood is based on the Planck 2015 data and considers both temperature and …

We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from
the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of …

… This Planck low-ℓ likelihood replaces the Planck temperature … WMAP 9-yr low-ℓ polarization
module used in the Planck 2013 … this Planck-only low-ℓ likelihood module, the basic Planck …

… ) and constraints on primordial non-Gaussianities (Planck Collaboration XVII 2016). In this
paper we use the 2015 data release from Planck 1 (Planck Collaboration I 2016) to … (9). As in …

… Planck Collaboration XX 2016). We have found no evidence for primordial non-Gaussianity
(… 9 The polarized synchrotron component is fitted only at 100GHz, being negligible at 143GHz…