Showing 1–20 of 60 results
/ Date/ Name
Jul 25, 2014The EAGLE project: Simulating the evolution and assembly of galaxies and their environmentsMar 11, 2022High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS projectJun 1, 2021Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer SimulationsOct 7, 2014SKIRT: an Advanced Dust Radiative Transfer Code with a User-Friendly ArchitectureMar 2, 2020SKIRT 9: redesigning an advanced dust radiative transfer code to allow kinematics, line transfer and polarization by aligned dust grainsMay 24, 2018The Failure of Monte Carlo Radiative Transfer at Medium to High Optical DepthsOct 7, 2013Using 3D Voronoi grids in radiative transfer simulationsDec 3, 2012FitSKIRT: genetic algorithms to automatically fit dusty galaxies with a Monte Carlo radiative transfer codeDec 15, 2017Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE projectJul 15, 2016Far-infrared and dust properties of present-day galaxies in the EAGLE simulationsJun 17, 2015Benchmarking the Calculation of Stochastic Heating and Emissivity of Dust Grains in the Context of Radiative Transfer SimulationsAug 12, 2022UV to submillimetre luminosity functions of TNG50 galaxiesJul 30, 2019Optical depth in polarised Monte Carlo radiative transferJul 5, 2021Polarised emission from aligned dust grains in nearby galaxies: predictions from the Auriga simulationsMay 5, 2017Optical colours and spectral indices of $z=0.1$ EAGLE galaxies with 3D dust radiative transfer code SKIRTJan 25, 2019The cosmic spectral energy distribution in the EAGLE simulationJun 13, 2023Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxiesAug 12, 2022Monte Carlo radiative transfer with explicit absorption to simulate absorption, scattering, and stimulated emissionDec 9, 2022Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at $z\sim 7$Jan 16, 2019The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation