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20112026
most citedPlanck 2015 results. XVII. Constraints on primordial non-Gaussianity

507 citations · 4.8k across the 27 of their papers we have counts for

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6 papers · 1 filter

astro-ph.CO2011★ 125 cited

Planck Early Results: Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue

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

The data reported in Planck's Early Release Compact Source Catalogue (ERCSC) are exploited to measure the number counts (dN/dS) of extragalactic radio sources at 30, 44, 70, 100, 1…

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★ 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).…

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 (…

astro-ph.CO2011★ 161 cited

Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates

Planck Collaboration, N. Aghanim, M. Arnaud +197

We present the XMM-Newton follow-up for confirmation of Planck cluster candidates. Twenty-five candidates have been observed to date using snapshot (~10 ksec) exposures, ten as par…