activity
20002018
most citedPlanck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps

263 citations · 837 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2018★ 99 cited

Planck 2018 results. II. Low Frequency Instrument data processing

Planck Collaboration, Y. Akrami, F. Argüeso +148

We present a final description of the data-processing pipeline for the Planck, Low Frequency Instrument (LFI), implemented for the 2018 data release. Several improvements have been…

astro-ph.CO2015★ 98 cited

Planck 2015 results. III. LFI systematic uncertainties

Planck Collaboration, P. A. R. Ade, J. Aumont +166

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…

astro-ph.GA2015★ 103 cited

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds

Planck Collaboration, P. A. R. Ade, N. Aghanim +238

(abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP. The Commander component-separation tool has been used to separate…

astro-ph.CO2015★ 55 cited

Planck 2015 results. VI. LFI mapmaking

Planck Collaboration, P. A. R. Ade, N. Aghanim +198

This paper describes the mapmaking procedure applied to Planck LFI (Low Frequency Instrument) data. The mapmaking step takes as input the calibrated timelines and pointing informat…

astro-ph.CO2015★ 263 cited

Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps

Planck Collaboration, R. Adam, P. A. R. Ade +223

This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperatur…

astro-ph.IM2015★ 74 cited

Planck 2015 results. VII. HFI TOI and beam processing

Planck Collaboration, R. Adam, P. A. R. Ade +225

The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polari…