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most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 41.7k across the 183 of their papers we have counts for

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astro-ph.GA2018★ 195 cited

Planck 2018 results. XII. Galactic astrophysics using polarized dust emission

Planck Collaboration, N. Aghanim, Y. Akrami +160

We present 353 GHz full-sky maps of the polarization fraction , angle , and dispersion of angles of Galactic dust thermal emission produced from the 2018 release of Planc…

astro-ph.GA2016★ 26 cited

Planck intermediate results. XLV. Radio spectra of northern extragalactic radio sources

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

Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on f…

astro-ph.GA2016★ 25 cited

Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap

Planck Collaboration, N. Aghanim, M. I. R. Alves +165

We study the statistical properties of interstellar dust polarization at high Galactic latitude, using the Stokes parameter Planck maps at 353 GHz. Our aim is to advance the unders…

astro-ph.GA2015★ 103 cited

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds

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

(abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP. The Commander component-separation tool has been used to separate…

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.GA2015★ 422 cited

Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Planck Collaboration, P. A. R. Ade, N. Aghanim +195

Within ten nearby (d < 450 pc) Gould Belt molecular clouds we evaluate statistically the relative orientation between the magnetic field projected on the plane of sky, inferred fro…

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.GA2014★ 69 cited

Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust

Planck Collaboration, R. Adam, P. A. R. Ade +199

The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic. The Planck all-sky maps of linearly pola…

astro-ph.GA2014★ 46 cited

Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck

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

The Andromeda Galaxy (M31) is one of a few galaxies that has sufficient angular size on the sky to be resolved by the Planck satellite. Planck has detected M31 in all of its freque…

astro-ph.GA2014★ 26 cited

Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data

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

Planck data when combined with ancillary data provide a unique opportunity to separate the diffuse emission components of the inner Galaxy. The purpose of the paper is to elucidate…

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★ 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.GA2012★ 70 cited

Planck Intermediate Results. IX. Detection of the Galactic haze with Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +181

Using precise full-sky observations from Planck, and applying several methods of component separation, we identify and characterize the emission from the Galactic "haze" at microwa…

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.GA2011★ 114 cited

Planck Early Results: The submillimetre properties of a sample of Galactic cold clumps

Planck Collaboration, P. A. R. Ade, N. Aghanim +201

(abridged) We perform a detailed investigation of sources from the Cold Cores Catalogue of Planck Objects (C3PO). Our goal is to probe the reliability of the detections, validate t…

astro-ph.GA2011★ 453 cited

Planck Early Results: All sky temperature and dust optical depth from Planck and IRAS: Constraints on the "dark gas" in our galaxy

Planck Collaboration, P. A. R. Ade, N. Aghanim +204

We construct an all-sky map of the apparent temperature and optical depth of thermal dust emission using the Planck-HFI and IRAS data. The optical depth maps are correlated to trac…

astro-ph.GA2011★ 117 cited

Planck early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources

Planck Collaboration, J. Aatrokoski, P. A. R. Ade +246

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact S…

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.GA2011★ 217 cited

Planck Early Results XXIV: Dust in the diffuse interstellar medium and the Galactic halo

Planck Collaboration, A. Abergel, P. A. R. Ade +205

This paper presents the first results of comparison of Planck along with IRAS data with Green Bank Telescope 21-cm observations in 14 fields covering more than 800 square degrees a…

astro-ph.GA2011★ 148 cited

Planck early results. XXI. Properties of the interstellar medium in the Galactic plane

Planck Collaboration, A. Abergel, P. A. R. Ade +199

(abridged) Planck has observed the entire sky from 30 GHz to 857GHz. The observed foreground emission contains contributions from different phases of the interstellar medium (ISM).…