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20082015
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 33.6k across the 87 of their papers we have counts for

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astro-ph.CO2015★ 38 cited

Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster

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

The Virgo cluster is the largest Sunyaev-Zeldovich (SZ) source in the sky, both in terms of angular size and total integrated flux. Planck's wide angular scale and frequency covera…

astro-ph.CO2015★ 80 cited

Planck 2013 results. XXXI. Consistency of the Planck data

Planck Collaboration, P. A. R. Ade, M. Arnaud +180

The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the compariso…

astro-ph.CO2015★ 146 cited

Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources

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

The Second Planck Catalogue of Compact Sources is a catalogue of sources detected in single-frequency maps from the full duration of the Planck mission and supersedes previous vers…

astro-ph.CO2015★ 39 cited

Planck Intermediate Results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes in the Canary Islands Observatories

Planck Collaboration, P. A. R. Ade, N. Aghanim +187

We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories as part of the gene…

astro-ph.CO2015★ 56 cited

Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +189

By looking at the kinetic Sunyaev-Zeldovich effect (kSZ) in Planck nominal mission data, we present a significant detection of baryons participating in large-scale bulk flows aroun…

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.CO2015★ 325 cited

Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources

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

We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of ga…

astro-ph.CO2015★ 10 cited

Planck 2015 results. XX. Constraints on inflation

Planck Collaboration, P. A. R. Ade, N. Aghanim +244

We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on 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★ 183 cited

Planck 2015 results. XXI. The integrated Sachs-Wolfe effect

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

This paper presents a study of the ISW effect from the Planck 2015 temperature and polarization data release. The CMB is cross-correlated with different LSS tracers: the NVSS, SDSS…

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★ 507 cited

Planck 2015 results. XVII. Constraints on primordial non-Gaussianity

Planck Collaboration, P. A. R. Ade, N. Aghanim +239

The Planck full mission cosmic microwave background(CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity(NG). Using three…

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★ 372 cited

Planck 2015 results. XIV. Dark energy and modified gravity

Planck Collaboration, P. A. R. Ade, N. Aghanim +232

We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG), beyond the cosmological constant scenario. We start with cases where the DE only…

astro-ph.CO2015★ 10.6k cited

Planck 2015 results. XIII. Cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +259

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary…

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.CO2014★ 222 cited

Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

Planck Collaboration, R. Adam, P. A. R. Ade +230

The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 1…

astro-ph.CO2014★ 57 cited

Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope

Planck Collaboration, P. A. R. Ade, N. Aghanim +194

We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with the Russian-Turkish 1.5-m telescope (RTT150), as a part of the opt…

astro-ph.CO2014★ 52 cited

Planck intermediate results. XXIV. Constraints on variation of fundamental constants

P. A. R. Ade, N. Aghanim, M. Arnaud +166

Any variation of the fundamental physical constants, and more particularly of the fine structure constant, , or of the mass of the electron, , would affect the recombinatio…

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.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.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…