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Planck 2015 results: XII. Full focal plane simulations in future updates. Generated at a cost of some 25 million CPU-hours spread across multiple high

Planck 2015 results: V. LFI calibration© 2016 ESO.We present a description of the pipeline used to calibrate the Planck Low Frequency

Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope-Zeldovich (SZ) sources with the Russian-Turkish 1.5 m telescope (RTT150), as a part of the optical follow

Planck intermediate results: XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories of them obtained with a multi-object spectroscopic mode. The sample contains new redshifts for 27 Planck

Planck 2015 results: II. Low Frequency Instrument data processings

Planck 2015 results: I. Overview of products and scientific results, including both temperature and polarization, along with a set of scientific and technical papers and a web

Planck 2015 results: XX. Constraints on inflation for the 2013 release papers. The Planck full mission temperature data and a first release of polarization data

Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts© 2014 ESO. We present constraints on cosmological parameters using number counts as a function

Planck intermediate results: XXXIX. the Planck list of high-redshift source candidates© ESO, 2016.The Planck mission, thanks to its large frequency range and all-sky coverage, has a

Planck intermediate results: XXV. the Andromeda galaxy as seen by Planck© ESO 2015. The Andromeda galaxy (M 31) is one of a few galaxies that has sufficient angular size

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