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19982025
most citedSecondary anisotropies of the CMB

90 citations · 808 across the 28 of their papers we have counts for

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Showing 2019Show all

13 papers · 1 filter

astro-ph.CO2019

Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects

V. Bonjean, N. Aghanim, M. Douspis +2

The role played by the large-scale structures in the galaxy evolution is not quite well understood yet. In this study, we investigate properties of galaxy in the range 0.1<z<0.3 fr…

astro-ph.CO2019

Probing the azimuthal environment of galaxies around clusters. From cluster core to cosmic filaments

C. Gouin, N. Aghanim, V. Bonjean +1

Galaxy clusters are connected at their peripheries to the large scale structures by cosmic filaments that funnel accreting material. These filamentary structures are studied to inv…

astro-ph.CO201950 cited

Like a spider in its web: a study of the Large Scale Structure around the Coma cluster

Nicola Malavasi, Nabila Aghanim, Hideki Tanimura +2

The Cosmic Web is a complex network of filaments, walls and voids that represent the largest structures in the Universe. In this network, which is the direct result of structure fo…

astro-ph.CO2019

Density and temperature of cosmic-web filaments on scales of tens of megaparsecs

H. Tanimura, N. Aghanim, V. Bonjean +2

We studied physical properties of matter in 24,544 filaments ranging from 30 to 100 Mpc in length, identified in the Sloan Digital Sky Survey (SDSS). We stacked the Comptonization…

astro-ph.CO2019

Microwave Spectro-Polarimetry of Matter and Radiation across Space and Time

Jacques Delabrouille, Maximilian H. Abitbol, Nabila Aghanim +77

This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-di…

astro-ph.CO2019

Planck 2018 results. V. CMB power spectra and likelihoods

Planck Collaboration, N. Aghanim, Y. Akrami +165

This paper describes the 2018 Planck CMB likelihoods, following a hybrid approach similar to the 2015 one, with different approximations at low and high multipoles, and implementin…