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Planck intermediate results: XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories

Planck 2015 results: V. LFI calibration

Planck 2015 results: II. Low Frequency Instrument data processings

Planck intermediate results: XLII. Large-scale Galactic magnetic fields

Planck 2015 results: XII. Full focal plane simulations

Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps about 1022 cm-2): Musca, B211, and L1506. These three filaments are detected above the background

Planck 2015 results: IV. Low Frequency Instrument beams and window functions uncertainties in the effective beam window functions are 0.7% and 1% at 30 and 44 GHz, respectively (at ≈ 600

Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps about 1022 cm-2): Musca, B211, and L1506. These three filaments are detected above the background

Planck 2015 results: XI. CMB power spectra, likelihoods, and robustness of parameters approach used for the previous release, i.e., a pixel-based likelihood at low multipoles ( < 30) and a

Planck 2015 results: XXV. Diffuse low-frequency Galactic foregrounds all the emission at 40deg > l >-90deg is part of the Loop I structure, and show that the emission

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