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19982026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 51.9k across the 321 of their papers we have counts for

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astro-ph.CO2020★ 77 cited

First detection of stacked X-ray emission from cosmic web filaments

H. Tanimura, N. Aghanim, A. Kolodzig +2

We report the first statistical detection of X-ray emission from cosmic web filaments in ROSAT data. We selected 15,165 filaments at 0.2<z<0.6 ranging from 30 Mpc to 100 Mpc in len…

astro-ph.CO2020★ 53 cited

Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear

M. Martinelli, I. Tutusaus, M. Archidiacono +91

Upcoming surveys will map the growth of large-scale structure with unprecented precision, improving our understanding of the dark sector of the Universe. Unfortunately, much of the…

astro-ph.GA2020★ 114 cited

Euclid preparation: X. The Euclid photometric-redshift challenge

Euclid Collaboration, G. Desprez, S. Paltani +170

Forthcoming large photometric surveys for cosmology require precise and accurate photometric redshift (photo-z) measurements for the success of their main science objectives. Howev…

astro-ph.CO2020★ 311 cited

Planck intermediate results. LVII. Joint Planck LFI and HFI data processing

Planck Collaboration, Y. Akrami, K. J. Andersen +136

We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High…

astro-ph.CO2020★ 10 cited

High resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations

Louis Legrand, Carlos Hernández-Monteagudo, Marian Douspis +2

In the context of next-generation spectroscopic galaxy surveys, new statistics of the distribution of matter are currently being developed. Among these, we investigated the angular…

astro-ph.CO2020★ 32 cited

Impact of systematics on cosmological parameters from future Galaxy Clusters surveys

Laura Salvati, Marian Douspis, Nabila Aghanim

Galaxy clusters are a recent cosmological probe. The precision and accuracy of the cosmological parameters inferred from these objects are affected by the knowledge of cluster phys…