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TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
Anand Utsav Kapoor, Maarten Baes, Arjen van der Wel +10
We present and publicly release a new star-forming regions emission library TODDLERS (Time evolution of Observables including Dust Diagnostics and Line Emission from Regions contai…
Self-consistent dust and non-LTE line radiative transfer with SKIRT
Kosei Matsumoto, Peter Camps, Maarten Baes +4
We introduce Monte Carlo-based non-LTE line radiative transfer calculations in the 3D dust radiative transfer code SKIRT, which was originally set up as a dust radiative transfer c…
Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
Daniela Barrientos Acevedo, Arjen van der Wel, Maarten Baes +6
We present a framework to build realistic mock spectroscopic observations for state-of-the-art hydrodynamical simulations, using high spectral resolution stellar population models…
X-ray radiative transfer in full 3D with SKIRT
Bert Vander Meulen, Peter Camps, Marko Stalevski +1
Models of active galactic nuclei (AGN) suggest that their circumnuclear media are complex with clumps and filaments, while recent observations hint towards polar extended structure…
Simulated observations of star formation regions: infrared evolution of globally collapsing clouds
Jesús M. Jáquez-Domínguez, Roberto Galván-Madrid, Jacopo Fritz +6
The direct comparison between hydrodynamical simulations and observations is needed to improve the physics included in the former and test biases in the latter. Post-processing rad…
The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
Andrea Gebek, Maarten Baes, Benedikt Diemer +6
Cold gas in galaxies provides a crucial test to evaluate the realism of cosmological hydrodynamical simulations. To extract the atomic and molecular hydrogen properties of the simu…