activity
20182024
most citedCharacterising filaments in the SDSS volume from the galaxy distribution

62 citations · 370 across the 12 of their papers we have counts for

collaborators
Showing 2019Show all

6 papers · 1 filter

astro-ph.CO2019★ 45 cited

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★ 8 cited

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.CO2019★ 18 cited

Deep learning for Sunyaev-Zel'dovich detection in Planck

Victor Bonjean

The Planck collaboration has extensively used the six Planck HFI frequency maps to detect the Sunyaev-Zel'dovich (SZ) effect with dedicated methods, e.g., by applying (i) component…

astro-ph.CO2019★ 50 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★ 57 cited

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.GA2019★ 54 cited

Star formation rates and stellar masses from machine learning

V. Bonjean, N. Aghanim, P. Salomé +3

Star-formation activity is a key property to probe the structure formation and hence characterise the large-scale structures of the universe. This information can be deduced from t…