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20112018
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 16k across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2018★ 203 cited

Planck 2018 results. XI. Polarized dust foregrounds

Planck Collaboration, Y. Akrami, M. Ashdown +131

The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic du…

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★ 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★ 10.6k cited

Planck 2015 results. XIII. Cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +259

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary…

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.GA2014★ 111 cited

Planck intermediate results. XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps

Planck Collaboration, P. A. R. Ade, N. Aghanim +187

Planck observations at 353GHz provide the first fully-sampled maps of the polarized dust emission towards interstellar filaments and their backgrounds. The polarization data provid…

astro-ph.GA2014★ 154 cited

Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations

Plank Collaboration, P. A. R. Ade, N. Aghanim +195

We present all-sky modelling of the high resolution Planck, IRAS, and WISE infrared (IR) observations using the physical dust model presented by Draine and Li in 2007 (DL). We stud…

astro-ph.CO2013★ 513 cited

Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +272

We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev--Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite o…

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.IM2013★ 97 cited

Planck 2013 results. II. Low Frequency Instrument data processing

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +229

We describe the data processing pipeline of the Planck Low Frequency Instrument (LFI) data processing centre (DPC) to create and characterize full-sky maps based on the first 15.5…

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.CO2012★ 203 cited

Planck Intermediate Results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +214

Taking advantage of the all-sky coverage and broad frequency range of the Planck satellite, we study the Sunyaev-Zeldovich (SZ) and pressure profiles of 62 nearby massive clusters…

astro-ph.CO2011★ 87 cited

Planck Early Results XXVI: Detection with Planck and confirmation by XMM-Newton of PLCK G266.6-27.3, an exceptionally X-ray luminous and massive galaxy cluster at z~1

Planck Collaboration, N. Aghanim, M. Arnaud +189

We present first results on PLCK G266.6-27.3, a galaxy cluster candidate detected at a signal-to-noise ratio of 5 in the Planck All Sky survey. An XMM-Newton validation observation…

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…