activity
19982015
most citedPlanck 2013 results. XI. All-sky model of thermal dust emission

827 citations · 5.2k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.CO2015★ 281 cited

Planck 2015 results. X. Diffuse component separation: Foreground maps

Planck Collaboration, R. Adam, P. A. R. Ade +236

Planck has mapped the microwave sky in nine frequency bands between 30 and 857 GHz in temperature and seven bands between 30 and 353 GHz in polarization. In this paper we consider…

astro-ph.GA2015★ 101 cited

Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold Clumps

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

We present the Planck Catalogue of Galactic Cold Clumps (PGCC), an all-sky catalogue of Galactic cold clump candidates detected by Planck. This catalogue is the full version of the…

astro-ph.CO2015★ 482 cited

Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts

Planck Collaboration, P. A. R. Ade, N. Aghanim +233

We present cluster counts and corresponding cosmological constraints from the Planck full mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev-Zeldov…

astro-ph.CO2015★ 172 cited

Planck 2015 results. XIX. Constraints on primordial magnetic fields

Planck Collaboration, P. A. R. Ade, N. Aghanim +230

We compute and investigate four types of imprint of a stochastic background of primordial magnetic fields (PMFs) on the cosmic microwave background (CMB) anisotropies: the impact o…

astro-ph.CO2015★ 87 cited

Planck 2015 results. XVIII. Background geometry & topology

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

Full-sky CMB maps from the 2015 Planck release allow us to detect departures from global isotropy on the largest scales. We present the first searches using CMB polarization for co…

astro-ph.CO2015★ 287 cited

Planck 2015 results. XV. Gravitational lensing

Planck Collaboration, P. A. R. Ade, N. Aghanim +227

We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40 sigma), using temperature and polarization data fro…

astro-ph.CO2015★ 99 cited

Planck 2015 results. IV. Low Frequency Instrument beams and window functions

Planck Collaboration, P. A. R. Ade, N. Aghanim +200

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). The stru…

astro-ph.GA2015★ 38 cited

Planck intermediate results. XXXIV. The magnetic field structure in the Rosette Nebula

Planck Collaboration, N. Aghanim, M. I. R. Alves +197

Planck has mapped the polarized dust emission over the whole sky, making it possible to trace the Galactic magnetic field structure that pervades the interstellar medium (ISM). We…

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…

astro-ph.IM2011★ 190 cited

Planck early results: first assessment of the High Frequency Instrument in-flight performance

Planck HFI Core Team, P. A. R. Ade, N. Aghanim +163

The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six w…

astro-ph.GA2011★ 201 cited

Planck Early Results: The Galactic Cold Core Population revealed by the first all-sky survey

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

We present the statistical properties of the first version of the Cold Core Catalogue of Planck Objects (C3PO), in terms of their spatial distribution, temperature, distance, mass,…

astro-ph.CO2011★ 119 cited

Planck early results: Cluster Sunyaev-Zeldovich optical scaling relations

Planck Collaboration, N. Aghanim, M. Arnaud +202

We present the Sunyaev-Zeldovich (SZ) signal-to-richness scaling relation (Y500-N200) for the MaxBCG cluster catalogue. Employing a multi-frequency matched filter on the Planck sky…

astro-ph.IM2011★ 88 cited

Planck Early Results. V. The Low Frequency Instrument data processing

A. Zacchei, D. Maino, C. Baccigalupi +146

We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discus…

astro-ph.GA2011★ 239 cited

Planck Early Results: Thermal dust in Nearby Molecular Clouds

Planck Collaboration, A. Abergel, P. A. R. Ade +197

Planck allows unbiased mapping of Galactic sub-millimetre and millimetre emission from the most diffuse regions to the densest parts of molecular clouds. We present an early analys…

astro-ph.CO2011★ 230 cited

Planck Early Results XVIII: The power spectrum of cosmic infrared background anisotropies

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 square degrees, we determine the angular power spectra of cosmic infrared background (…