activity
20042023
most citedGALICS -- VI. Modelling Hierarchical Galaxy Formation in Clusters

66 citations · 113 across the 6 of their papers we have counts for

collaborators

6 papers

math.AP2023

Scattered wavefield in the stochastic homogenization regime

Josselin Garnier, Laure Giovangigli, Quentin Goepfert +1

In the context of providing a mathematical framework for the propagation of ultrasound waves in a random multiscale medium, we consider the scattering of classical waves (modeled b…

astro-ph.HE2021★ 11 cited

Limit on intergalactic magnetic field from ultra-high-energy cosmic ray hotspot in Perseus-Pisces region

Andrii Neronov, Dmitri Semikoz, Oleg Kalashev

Telescope Array collaboration has reported an evidence for existence of a source of ultra-high-energy cosmic ray (UHECR) events in Perseus-Pisces supercluster. We show that the mer…

physics.ins-det2020★ 18 cited

SND@LHC

SHiP Collaboration, C. Ahdida, A. Akmete +341

We propose to build and operate a detector that, for the first time, will measure the process at the LHC and search for feebly interacting particles (FIPs) in an unexplor…

astro-ph2008★ 2 cited

Properties and Chemical Evolution of the M31 Disk: Comparison with the Milky Way

J. L. Hou, J. Yin, S. Boissier +3

By adopting the chemical evolution model of the Milky Way disk, we have studied the star formation and chemical evolution history for M31 galaxy disk. We mainly concentrated on the…

astro-ph2005★ 66 cited

GALICS -- VI. Modelling Hierarchical Galaxy Formation in Clusters

B. Lanzoni, B. Guiderdoni, G. A. Mamon +2

High-resolution N-body re-simulations of 15 massive (10^{14}-10^{15} Msun) dark matter haloes have been combined with the hybrid galaxy formation model GalICS (Hatton et al. 2003),…

astro-ph2004★ 16 cited

FUSE search for 10^5-10^6 K gas in the rich clusters of galaxies Abell 2029 and Abell 3112

A. Lecavelier des Etangs, Gopal-Krishna, F. Durret

Recent Chandra and XMM X-ray observations of rich clusters of galaxies have shown that the amount of hot gas which is cooling below ~1 keV is generally more modest than previous es…