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Effects of dust sources on dust attenuation properties in IllustrisTNG galaxies at
Yuan-Ming Hsu, Hiroyuki Hirashita, Yen-Hsing Lin +2
Dust emission from high-redshift galaxies gives us a clue to the origin and evolution of dust in the early Universe. Previous studies have shown that different sources of dust (ste…
UV to submillimetre luminosity functions of TNG50 galaxies
Ana Trcka, Maarten Baes, Peter Camps +7
We apply the radiative transfer (RT) code SKIRT on a sample of ~14000 low-redshift (z<= 0.1) galaxies extracted from the TNG50 simulation to enable an apples-to-apples comparison w…
Monte Carlo radiative transfer with explicit absorption to simulate absorption, scattering, and stimulated emission
Maarten Baes, Peter Camps, Kosei Matsumoto
Context: The Monte Carlo method is probably the most widely used approach to solve the radiative transfer problem, especially in a general 3D geometry. The physical processes of em…
High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
Peter Camps, Anand Utsav Kapoor, Ana Trčka +4
We present redshift-zero synthetic dust-aware observations for the 45 Milky Way-mass simulated galaxies of the ARTEMIS project, calculated with the SKIRT radiative transfer code. T…
A new analytical scattering phase function for interstellar dust
Maarten Baes, Peter Camps, Anand Utsav Kapoor
Context: Properly modelling scattering by interstellar dust grains requires a good characterisation of the scattering phase function. The Henyey-Greenstein phase function has becom…