G. Roudier

TL;DR: The NPIPE pipeline as mentioned in this paper produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and high frequency instrument (HFI) using high-performance computers.

TL;DR: The Planck Multi-frequency Catalogue of Non-thermal (PCNT) as discussed by the authors was constructed by selecting objects detected in the full mission all-sky temperature maps at 30 and 143 GHz, with a signal-to-noise ratio (S/N)> 3 in at least one of the two channels after filtering with a particular Mexican hat wavelet.

TL;DR: In this paper, the authors presented a continuous spectrum covering centimetre to submillimetre wavelengths for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on four-epoch Planck data.

TL;DR: The Planck Multi-frequency Catalogue of Non-thermal (i.e. synchrotron-dominated) Sources (PCNT) observed between 30 and 857 GHz by the ESA Planck mission was constructed by selecting objects detected in the full-sky temperature maps at 30 and 143 GHz, with a signal-to-noise ratio (S/N)>3 in at least one of the two channels after filtering with a particular Mexican hat wavelet as discussed by the authors.

TL;DR: In this article, the authors used the Planck data to investigate the behaviour of zodiacal emission over the whole sky at sub-millimetre and millimetre wavelengths, finding the emissivities of the various components of the COBE zodiacAL model -- a diffuse cloud, three asteroidal dust bands, a circumsolar ring, and an Earth-trailing feature.