Showing 1–20 of 33 results
/ Date/ Name
Aug 11, 2019Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel'dovich approximationSep 2, 2008Numerical simulations of buoyancy instabilities in galaxy cluster plasmas with cosmic rays and anisotropic thermal conductionOct 8, 2019Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe RunsMay 23, 2005The History of the Baryon Budget: Cosmic Logistics in a Hierarchical UniverseJun 5, 2019Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster SamplesNov 22, 2013Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR $Λ$CDM simulationSep 1, 2008Abundance profiles in cooling-core clusters: a fossil record of past AGN-driven convection?Jul 29, 2005Soft gamma-ray background and light Dark Matter annihilationMar 12, 2018Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scalesApr 16, 2026PySCo-EFT and ECOSMOG-EFT: a tandem of N-body simulation codes for the Effective Field Theory of Dark EnergyNov 13, 2019Phase-space structure of cold dark matter halos inside splashback: multi-stream flows and self-similar solutionMay 26, 2014Probing dark energy models with extreme pairwise velocities of galaxy clusters from the DEUS-FUR simulationsOct 3, 2018The environmental dependence of the baryon acoustic peak in the Baryon Oscillation Spectroscopic Survey CMASS sampleJul 29, 2020Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR $Cosmo$ SimulationsSep 13, 2021Detectability of the gravitational redshift effect from the asymmetric galaxy clusteringMar 15, 2023The e-MANTIS emulator: fast predictions of the non-linear matter power spectrum in $f(R)$CDM cosmologyDec 2, 2014Small scale clustering of late forming dark matterJul 16, 2007Convection and AGN Feedback in Clusters of GalaxiesDec 14, 2021Cosmological test of local position invariance from the asymmetric galaxy clusteringFeb 11, 2022The short ionizing photon mean free path at z=6 in Cosmic Dawn III, a new fully-coupled radiation-hydrodynamical simulation of the Epoch of Reionization