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19992015
most citedPlanck 2015 results. XVII. Constraints on primordial non-Gaussianity

507 citations · 2.5k across the 15 of their papers we have counts for

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9 papers · 1 filter

astro-ph.CO2015★ 79 cited

Planck 2015 results. XII. Full Focal Plane simulations

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

We present the 8th Full Focal Plane simulation set (FFP8), deployed in support of the Planck 2015 results. FFP8 consists of 10 fiducial mission realizations reduced to 18144 maps,…

astro-ph.CO2015★ 80 cited

Planck 2013 results. XXXI. Consistency of the Planck data

Planck Collaboration, P. A. R. Ade, M. Arnaud +180

The Planck design and scanning strategy provide many levels of redundancy that can be exploited to provide tests of internal consistency. One of the most important is the compariso…

astro-ph.CO2015★ 428 cited

Planck 2015 results. XVI. Isotropy and statistics of the CMB

Planck Collaboration, P. A. R. Ade, N. Aghanim +242

We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly…

astro-ph.CO2015★ 276 cited

Planck 2015 results. IX. Diffuse component separation: CMB maps

Planck Collaboration, R. Adam, P. A. R. Ade +236

We present foreground-reduced CMB maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature sky maps, t…

astro-ph.CO2015★ 507 cited

Planck 2015 results. XVII. Constraints on primordial non-Gaussianity

Planck Collaboration, P. A. R. Ade, N. Aghanim +239

The Planck full mission cosmic microwave background(CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity(NG). Using three…

astro-ph.CO2014★ 222 cited

Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

Planck Collaboration, R. Adam, P. A. R. Ade +230

The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 1…

astro-ph.CO2013★ 395 cited

Planck 2013 results. XVII. Gravitational lensing by large-scale structure

Planck Collaboration, P. A. R. Ade, N. Aghanim +235

On the arcminute angular scales probed by Planck, the CMB anisotropies are gently perturbed by gravitational lensing. Here we present a detailed study of this effect, detecting len…

astro-ph.CO2013★ 65 cited

Planck 2013 results. III. LFI systematic uncertainties

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +217

We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological…

astro-ph.CO2011★ 47 cited

Planck Intermediate Results. I. Further validation of new Planck clusters with XMM-Newton

The Planck Collaboration, N. Aghanim, M. Arnaud +182

We present further results from the ongoing XMM-Newton validation follow-up of Planck cluster candidates, detailing X-ray observations of eleven candidates detected at a signal-to-…