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20002013
most citedPlanck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample

413 citations · 2.5k across the 11 of their papers we have counts for

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Showing 2011Show all

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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.CO2011★ 151 cited

Planck Early Results: Origin of the submm excess dust emission in the Magellanic Clouds

Planck Collaboration, P. A. R. Ade, N. Aghanim +197

The integrated Spectral Energy Distributions of the Large and Small Magellanic Cloud appear significantly flatter than expected from dust models based on their FIR and radio emissi…

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…