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most citedPlanck 2013 results. XVI. Cosmological parameters

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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.CO2013★ 305 cited

Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation

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

We present new measurements of CIB anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross frequency power spectrum is measured from 143 to 3000 GHz, a…

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★ 577 cited

Planck 2013 results. XV. CMB power spectra and likelihood

Planck collaboration, P. A. R. Ade, N. Aghanim +257

We present the Planck likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations. We use this likelihood to derive the…

astro-ph.GA2013★ 221 cited

Planck 2013 results. XIII. Galactic CO emission

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

Rotational transition lines of CO play a major role in molecular radio astronomy and in particular in the study of star formation and the Galactic structure. Although a wealth of d…

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★ 293 cited

Planck 2013 results. XII. Component separation

Planck Collaboration, P. A. R. Ade, N. Aghanim +252

Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwav…

astro-ph.CO2013★ 61 cited

Planck intermediate results. XIII. Constraints on peculiar velocities

Planck Collaboration, P. A. R. Ade, N. Aghanim +182

Using \Planck\ data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we address the study of peculiar motions by searching for evidence of the kineti…

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★ 241 cited

Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +176

Our velocity relative to the rest frame of the cosmic microwave background (CMB) generates a dipole temperature anisotropy on the sky which has been well measured for more than 30…

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★ 1.1k cited

Planck 2013 results. XXII. Constraints on inflation

Planck Collaboration, P. A. R. Ade, N. Aghanim +241

We analyse the implications of the Planck data for cosmic inflation. The Planck nominal mission temperature anisotropy measurements, combined with the WMAP large-angle polarization…

astro-ph.CO2013★ 107 cited

Planck 2013 results. XXI. All-sky Compton parameter power spectrum and high-order statistics

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

We have constructed the first all-sky map of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 100 to 857 GHz freq…

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.CO2013★ 6.6k cited

Planck 2013 results. XVI. Cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +261

We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The Planck spectra at high multipoles are extremely well descr…

astro-ph.CO2013★ 128 cited

Planck 2013 results. XIV. Zodiacal emission

Planck Collaboration, P. A. R. Ade, N. Aghanim +229

The Planck satellite provides a set of all-sky maps at nine frequencies from 30 GHz to 857 GHz. Planets, minor bodies, and diffuse interplanetary dust emission (IPD) are all observ…

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.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…