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19992022
most citedPlanck 2013 results. I. Overview of products and scientific results

1.8k citations · 5.7k across the 25 of their papers we have counts for

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17 papers · 1 filter

astro-ph.CO2016★ 178 cited

Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters

Planck Collaboration, N. Aghanim, Y. Akrami +150

The six parameters of the standard CDM model have best-fit values derived from the Planck temperature power spectrum that are shifted somewhat from the best-fit values derived f…

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.CO2016★ 235 cited

Planck intermediate results. XLVII. Planck constraints on reionization history

Planck Collaboration, R. Adam, N. Aghanim +163

We investigate constraints on cosmic reionization extracted from the Planck cosmic microwave background (CMB) data. We combine the Planck CMB anisotropy data in temperature with th…

astro-ph.CO2016★ 25 cited

Planck intermediate results. XLIII. The spectral energy distribution of dust in clusters of galaxies

Planck Collaboration, R. Adam, P. A. R. Ade +177

Although infrared (IR) overall dust emission from clusters of galaxies has been statistically detected using data from the Infrared Astronomical Satellite (IRAS), it has not been p…

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★ 40 cited

Planck intermediate results. XVI. Profile likelihoods for cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +180

We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Minuit). This allows a refinement of the Lambda-cdm best-fit solution with respect…

astro-ph.CO2013★ 7 cited

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): A White Paper on the Ultimate Polarimetric Spectro-Imaging of the Microwave and Far-Infrared Sky

PRISM Collaboration, Philippe Andre, Carlo Baccigalupi +101

PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in response to the Call for White Papers for the definition of the L2 and L3 Missions in the ESA Sc…

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★ 625 cited

Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts

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

We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ…

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.CO2012★ 98 cited

Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies

Planck Collaboration, P. A. R. Ade, N. Aghanim +194

We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Surv…

astro-ph.CO2012★ 39 cited

Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz

Planck Collaboration, P. A. R. Ade, N. Aghanim +188

(abridged for arXiv) We make use of the Planck all-sky survey to derive number counts and spectral indices of extragalactic sources -- infrared and radio sources -- from the Planck…

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.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…

astro-ph.CO2009★ 258 cited

Improved measurements of the temperature and polarization of the CMB from QUaD

The QUaD collaboration, M. L. Brown, P. Ade +29

We present an improved analysis of the final dataset from the QUaD experiment. Using an improved technique to remove ground contamination, we double the effective sky area and henc…