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20112016
most citedPlanck 2013 results. I. Overview of products and scientific results

1.8k citations · 3.4k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2016★ 65 cited

Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB -mode analysis

Planck Collaboration, N. Aghanim, M. Ashdown +156

The characterization of the Galactic foregrounds has been shown to be the main obstacle in the challenging quest to detect primordial B-modes in the polarized microwave sky. We mak…

astro-ph.CO2015★ 40 cited

Planck 2015 results. I. Overview of products and scientific results

Planck Collaboration, R. Adam, P. A. R. Ade +352

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

astro-ph.CO2013★ 563 cited

Planck 2013 results. XXIII. Isotropy and statistics of the CMB

Planck Collaboration, P. A. R. Ade, N. Aghanim +252

The two fundamental assumptions of the standard cosmological model - that the initial fluctuations are statistically isotropic and Gaussian - are rigorously tested using maps of th…

astro-ph.CO2013★ 1.8k cited

Planck 2013 results. I. Overview of products and scientific results

Planck Collaboration, P. A. R. Ade, N. Aghanim +398

The ESA's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sk…

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.CO2011★ 150 cited

Planck early results. VI. The High Frequency Instrument data processing

Planck HFI Core Team, P. A. R. Ade, N. Aghanim +163

We describe the processing of the 336 billion raw data samples from the High Frequency Instrument (HFI) which we performed to produce six temperature maps from the first 295 days o…

astro-ph.CO2011★ 156 cited

Planck Early Results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters

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

All-sky data from the Planck survey and the Meta-Catalogue of X-ray detected Clusters of galaxies (MCXC) are combined to investigate the relationship between the thermal Sunyaev-Ze…

astro-ph.CO2011★ 283 cited

Planck Early Results. VII. The Early Release Compact Source Catalog

Planck Collaboration, P. A. R. Ade, N. Aghanim +228

(Abridged) A brief description of the methodology of construction, contents and usage of the Planck Early Release Compact Source Catalogue (ERCSC), including the Early Cold Cores (…

astro-ph.IM2011★ 143 cited

Planck Early Results. II. The thermal performance of Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +225

The performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative…

astro-ph.CO2011★ 83 cited

Planck early results XIV: ERCSC validation and extreme radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +206

Planck's all sky surveys at 30-857 GHz provide an unprecedented opportunity to follow the radio spectra of a large sample of extragalactic sources to frequencies 2-20 times higher…