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20052025
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 30.8k across the 95 of their papers we have counts for

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Showing astro-ph.GAShow all

21 papers · 1 filter

astro-ph.GA2025

Cross-correlations between X-ray clusters and the general galaxy population

Johan Comparat, Juan Macias-Perez, Céline Combet +5

This study presents highly precise measurements of the cross-correlation between volume-limited galaxy samples from the DESI legacy survey catalogue and X-ray selected galaxy clust…

astro-ph.GA2018★ 195 cited

Planck 2018 results. XII. Galactic astrophysics using polarized dust emission

Planck Collaboration, N. Aghanim, Y. Akrami +160

We present 353 GHz full-sky maps of the polarization fraction , angle , and dispersion of angles of Galactic dust thermal emission produced from the 2018 release of Planc…

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.GA2016★ 25 cited

Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap

Planck Collaboration, N. Aghanim, M. I. R. Alves +165

We study the statistical properties of interstellar dust polarization at high Galactic latitude, using the Stokes parameter Planck maps at 353 GHz. Our aim is to advance the unders…

astro-ph.GA2016★ 37 cited

Planck intermediate results. XLII. Large-scale Galactic magnetic fields

Planck Collaboration, R. Adam, P. A. R. Ade +175

Recent models for the large-scale Galactic magnetic fields in the literature have been largely constrained by synchrotron emission and Faraday rotation measures. We use three diffe…

astro-ph.GA2015★ 103 cited

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds

Planck Collaboration, P. A. R. Ade, N. Aghanim +238

(abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP. The Commander component-separation tool has been used to separate…