We present an update to the framework called Simulator of Galaxy Millimeter/submillimeter Emission (sígame). sígame derives line emission in the far-infrared (FIR) for galaxies in particle-based cosmological hydrodynamics simulations by applying radiative transfer and physics recipes via a postprocessing step after completion of the simulation. In this version, a new technique is developed to model higher gas densities by parameterizing the probability distribution function (PDF) of the gas density in higher-resolution simulations run with the pseudo-Lagrangian, Voronoi mesh code arepo. The parameterized PDFs are used as a look-up table, and reach higher densities than in previous work. sígame v3 is tested on redshift z = 0 galaxies drawn f...
The advent of new sub-millimetre (sub-mm) observational facilities has stimulated the desire to mode...
Context. The spectral energy distributions (SEDs) of low-mass low-metallicity (dwarf) galaxies are a...
We present full-volume cosmological simulations, using the moving-mesh code arepo to study the coevo...
We present an update to the framework called Simulator of Galaxy Millimeter/submillimeter Emission (...
Modelling galaxy formation in a cosmological context is challenging due to many physical processes a...
Atomic fine structure lines have been detected in the local Universe and at high redshifts over the ...
An updated version of the dust radiation transfer code sunrise, including mod-els for star-forming r...
Integral field observations of galaxies now produce spatially resolved emission line diagnostic diag...
Far-infrared (FIR) emission lines are a powerful tool to investigate the properties of the interstel...
International audienceA code computing consistently the evolution of stars, gas and dust, as well as...
Nebular line emission diagnostics have been instrumental in studying the galaxy properties over the ...
What main mechanisms set the star formation rate (SFR) of galaxies? This PhD thesis is a quest into ...
We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated...
International audienceInfrared and nebular lines provide some of our best probes of the physics regu...
Far-infrared molecular emission is an important tool used to understand the excitation mechanisms of...
The advent of new sub-millimetre (sub-mm) observational facilities has stimulated the desire to mode...
Context. The spectral energy distributions (SEDs) of low-mass low-metallicity (dwarf) galaxies are a...
We present full-volume cosmological simulations, using the moving-mesh code arepo to study the coevo...
We present an update to the framework called Simulator of Galaxy Millimeter/submillimeter Emission (...
Modelling galaxy formation in a cosmological context is challenging due to many physical processes a...
Atomic fine structure lines have been detected in the local Universe and at high redshifts over the ...
An updated version of the dust radiation transfer code sunrise, including mod-els for star-forming r...
Integral field observations of galaxies now produce spatially resolved emission line diagnostic diag...
Far-infrared (FIR) emission lines are a powerful tool to investigate the properties of the interstel...
International audienceA code computing consistently the evolution of stars, gas and dust, as well as...
Nebular line emission diagnostics have been instrumental in studying the galaxy properties over the ...
What main mechanisms set the star formation rate (SFR) of galaxies? This PhD thesis is a quest into ...
We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated...
International audienceInfrared and nebular lines provide some of our best probes of the physics regu...
Far-infrared molecular emission is an important tool used to understand the excitation mechanisms of...
The advent of new sub-millimetre (sub-mm) observational facilities has stimulated the desire to mode...
Context. The spectral energy distributions (SEDs) of low-mass low-metallicity (dwarf) galaxies are a...
We present full-volume cosmological simulations, using the moving-mesh code arepo to study the coevo...