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19952020
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 27.3k across the 140 of their papers we have counts for

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astro-ph.CO2020★ 311 cited

Planck intermediate results. LVII. Joint Planck LFI and HFI data processing

Planck Collaboration, Y. Akrami, K. J. Andersen +136

We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High…

astro-ph.CO2020★ 32 cited

Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II

Planck Collaboration, Y. Akrami, M. Ashdown +126

The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularl…

astro-ph.CO2019★ 39 cited

Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time

Jacques Delabrouille, Maximilian H. Abitbol, Nabila Aghanim +77

This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-di…

astro-ph.CO2019★ 1.1k cited

Planck 2018 results. V. CMB power spectra and likelihoods

Planck Collaboration, N. Aghanim, Y. Akrami +165

This paper describes the 2018 Planck CMB likelihoods, following a hybrid approach similar to the 2015 one, with different approximations at low and high multipoles, and implementin…

astro-ph.CO2019★ 159 cited

Planck 2018 results. IX. Constraints on primordial non-Gaussianity

Planck Collaboration, Y. Akrami, F. Arroja +157

We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare e…

astro-ph.CO2019★ 1 cited

Polarisation as a tracer of CMB anomalies: Planck results and future forecasts

M. Billi, A. Gruppuso, N. Mandolesi +2

The lack of power anomaly is an intriguing feature at the largest angular scales of the CMB anisotropy temperature pattern, whose statistical significance is not strong enough to c…

astro-ph.CO2018★ 2.4k cited

Planck 2018 results. X. Constraints on inflation

Planck Collaboration, Y. Akrami, F. Arroja +173

We report on the implications for cosmic inflation of the 2018 Release of the Planck CMB anisotropy measurements. The results are fully consistent with the two previous Planck cosm…

astro-ph.CO2018★ 745 cited

Planck 2018 results. VIII. Gravitational lensing

Planck Collaboration, N. Aghanim, Y. Akrami +155

We present measurements of the cosmic microwave background (CMB) lensing potential using the final 2018 temperature and polarization data. We increase the signifi…

astro-ph.CO2018★ 1.7k cited

Planck 2018 results. I. Overview and the cosmological legacy of Planck

Planck Collaboration, Y. Akrami, F. Arroja +188

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave…

astro-ph.CO2017★ 19 cited

Exploring cosmic origins with CORE: mitigation of systematic effects

P. Natoli, M. Ashdown, R. Banerji +123

We present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission. We employ timeline-to-map simulati…

astro-ph.CO2017★ 10 cited

Planck intermediate results. LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect

Planck Collaboration, N. Aghanim, Y. Akrami +141

Using the full-mission data, we present a detection of the temperature (and therefore velocity) dispersion due to the kinetic Sunyaev-Zeldovich (kSZ) effect from clu…

astro-ph.CO2017★ 24 cited

Exploring cosmic origins with CORE: effects of observer peculiar motion

C. Burigana, C. S. Carvalho, T. Trombetti +116

We discuss the effects on the CMB, CIB, and thermal SZ effect due to the peculiar motion of an observer with respect to the CMB rest frame, which induces boosting effects. We inves…

astro-ph.CO2016★ 18 cited

On the impact of large angle CMB polarization data on cosmological parameters

Massimiliano Lattanzi, Carlo Burigana, Martina Gerbino +6

(abridged) We study the impact of the large-angle CMB polarization datasets publicly released by the WMAP and Planck satellites on the estimation of cosmological parameters of the…

astro-ph.CO2016

The Planck legacy - Reinforcing the case for a standard model of cosmology: CDM

Nazzareno Mandolesi, Diego Molinari, Alessandro Gruppuso +2

We present a brief review of the main results of the Planck 2015 release describing the new calibration of the data, showing the maps delivered in temperature and, for the first ti…

astro-ph.CO2016★ 69 cited

Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies

Planck Collaboration, N. Aghanim, M. Ashdown +157

Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we imple…

astro-ph.CO2016★ 27 cited

Planck intermediate results. XLIX. Parity-violation constraints from polarization data

Planck Collaboration, N. Aghanim, M. Ashdown +148

Parity violating extensions of the standard electromagnetic theory cause in vacuo rotation of the plane of polarization of propagating photons. This effect, also known as cosmic bi…

astro-ph.CO2015★ 18 cited

Planck intermediate results. XLI. A map of lensing-induced B-modes

Planck Collaboration, P. A. R. Ade, N. Aghanim +178

The secondary cosmic microwave background (CMB) -modes stem from the post-decoupling distortion of the polarization -modes due to the gravitational lensing effect of large-sc…

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★ 10 cited

Pre-Inflationary Relics in the CMB?

A. Gruppuso, N. Kitazawa, N. Mandolesi +2

String Theory and Supergravity allow, in principle, to follow the transition of the inflaton from pre-inflationary fast roll to slow roll. This introduces an infrared depression in…

astro-ph.CO2015★ 98 cited

Planck 2015 results. III. LFI systematic uncertainties

Planck Collaboration, P. A. R. Ade, J. Aumont +166

We present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results…

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…