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most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 12.4k across the 38 of their papers we have counts for

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astro-ph.CO2015★ 663 cited

BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array

Keck Array, BICEP2 Collaborations, : +60

We present results from an analysis of all data taken by the BICEP2 & Keck Array CMB polarization experiments up to and including the 2014 observing season. This includes the first…

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.GA2015★ 26 cited

Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates

Planck Collaboration, P. A. R. Ade, N. Aghanim +186

The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources o…

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.GA2015★ 27 cited

Planck intermediate results. XXXVIII. E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium

Planck Collaboration, P. A. R. Ade, N. Aghanim +192

The quest for a B-mode imprint from primordial gravity waves on the polarization of the cosmic microwave background (CMB) requires the characterization of foreground polarization f…

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★ 10 cited

Planck 2015 results. XX. Constraints on inflation

Planck Collaboration, P. A. R. Ade, N. Aghanim +244

We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the…

astro-ph.CO2015★ 183 cited

Planck 2015 results. XXI. The integrated Sachs-Wolfe effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +229

This paper presents a study of the ISW effect from the Planck 2015 temperature and polarization data release. The CMB is cross-correlated with different LSS tracers: the NVSS, SDSS…

astro-ph.CO2015★ 263 cited

Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps

Planck Collaboration, R. Adam, P. A. R. Ade +223

This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperatur…

astro-ph.IM2015★ 74 cited

Planck 2015 results. VII. HFI TOI and beam processing

Planck Collaboration, R. Adam, P. A. R. Ade +225

The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polari…

astro-ph.IM2015★ 62 cited

Planck 2015 results. II. Low Frequency Instrument data processing

Planck Collaboration, P. A. R. Ade, N. Aghanim +213

We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our re…

astro-ph.IM2015★ 64 cited

BICEP2 III: Instrumental Systematics

BICEP2 Collaboration, P. A. R. Ade, R. W. Aikin +42

In a companion paper we have reported a detection of degree scale -mode polarization at 150 GHz by the BICEP2 experiment. Here we provide a detailed study of potential in…