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most citedPlanck 2013 results. XI. All-sky model of thermal dust emission

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astro-ph.GA2013★ 827 cited

Planck 2013 results. XI. All-sky model of thermal dust emission

Planck Collaboration, A. Abergel, P. A. R. Ade +244

This paper presents an all-sky model of dust emission from the Planck 857, 545 and 353 GHz, and IRAS 100 micron data. Using a modified black-body fit to the data we present all-sky…

astro-ph.CO2013★ 167 cited

Planck 2013 results. XVIII. Gravitational lensing-infrared background correlation

Planck Collaboration, P. A. R. Ade, N. Aghanim +223

The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the…

astro-ph.CO2013★ 210 cited

Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +240

The Planck Catalogue of Compact Sources (PCCS) is the catalogue of sources detected in the first 15 months of Planck operations, the "nominal" mission. It consists of nine single-f…

astro-ph.CO2013★ 133 cited

Planck 2013 results. XXVI. Background geometry and topology of the Universe

Planck Collaboration, P. A. R. Ade, N. Aghanim +223

Planck CMB temperature maps allow detection of large-scale departures from homogeneity and isotropy. We search for topology with a fundamental domain nearly intersecting the last s…

astro-ph.CO2013★ 457 cited

Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity

Planck Collaboration, P. A. R. Ade, N. Aghanim +237

The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG). Using three optimal bispectrum estimators, sep…

astro-ph.CO2013★ 91 cited

Planck 2013 results X. Energetic particle effects: characterization, removal, and simulation

Planck Collaboration, P. A. R. Ade, N. Aghanim +211

We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the \Planck\ High Frequency Instrument (HFI). There a…

astro-ph.CO2013★ 143 cited

Planck 2013 results. VIII. HFI photometric calibration and mapmaking

Planck Collaboration, P. A. R. Ade, N. Aghanim +223

This paper describes the processing applied to the HFI cleaned time-ordered data to produce photometrically calibrated maps. HFI observes the sky over a broad range of frequencies,…

astro-ph.CO2013★ 138 cited

Planck 2013 results. VI. High Frequency Instrument data processing

Planck Collaboration, P. A. R. Ade, N. Aghanim +235

We describe the processing of the 531 billion raw data samples from the High Frequency Instrument (hereafter HFI), which we performed to produce six temperature maps from the first…

astro-ph.IM2013★ 78 cited

Planck 2013 results. V. LFI calibration

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +217

We discuss the methods employed to photometrically calibrate the data acquired by the Low Frequency Instrument on Planck. Our calibration is based on a combination of the Orbital D…

astro-ph.CO2013★ 60 cited

Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +207

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). Knowledge…