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19982022
most citedPlanck 2018 results. X. Constraints on inflation

2.4k citations · 16.9k across the 85 of their papers we have counts for

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Showing 2013Show all

17 papers · 1 filter

astro-ph.GA2013★ 177 cited

Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies

Planck Collaboration, A. Abergel, P. A. R. Ade +196

The dust-HI correlation is used to characterize the emission properties of dust in the diffuse interstellar medium. We cross-correlate sky maps from Planck, WMAP, and DIRBE, at 17…

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.GA2013★ 5 cited

Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds

Planck Collaboration, P. A. R. Ade, N. Aghanim +180

Anomalous microwave emission (AME) is believed to be due to electric dipole radiation from small spinning dust grains. The aim of this paper is a statistical study of the basic pro…

astro-ph.GA2013★ 80 cited

Planck intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane

Planck Collaboration, P. A. R. Ade, N. Aghanim +190

We use Planck HFI data combined with ancillary radio data to study the emissivity index of the interstellar dust emission in the frequency range 10 - 353 GHz, or 3 - 0.8 mm, in the…

astro-ph.CO2013★ 346 cited

Planck 2013 results. XXV. Searches for cosmic strings and other topological defects

Planck Collaboration, P. A. R. Ade, N. Aghanim +225

Planck data have been used to provide stringent new constraints on cosmic strings and other defects. We describe forecasts of the CMB power spectrum induced by cosmic strings, calc…

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★ 513 cited

Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +272

We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev--Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite o…

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★ 159 cited

Planck 2013 results. XIX. The integrated Sachs-Wolfe effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +245

Based on CMB maps from the 2013 Planck Mission data release, this paper presents the detection of the ISW effect, i.e., the correlation between the CMB and large-scale evolving gra…

astro-ph.IM2013★ 188 cited

Planck 2013 results. IX. HFI spectral response

Planck Collaboration, P. A. R. Ade, N. Aghanim +217

The Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground based tests conducted with the HFI focal plane in a cryogenic environment pri…

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.IM2013★ 111 cited

Planck 2013 results. VII. HFI time response and beams

Planck Collaboration, P. A. R. Ade, N. Aghanim +220

This paper characterizes the effective beams,the effective beam window functions and the associated errors for the Planck HFI detectors. The effective beam is the angular response…

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.GA2013★ 26 cited

Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System

Planck Collaboration, P. A. R. Ade, N. Aghanim +179

We perform an analysis of the diffuse low-frequency Galactic components in the Southern part of the Gould Belt system (130^\circ\leq l\leq 230^\circ and -50^\circ\leq b\leq -10^\ci…