Infrared luminosity functions and dust mass functions in the EAGLE simulation
dc.contributor.author | Marchetti, Lucia | |
dc.contributor.author | Baes, Maarten | |
dc.contributor.author | Trcka, Ana | |
dc.date.accessioned | 2021-02-10T07:05:30Z | |
dc.date.available | 2021-02-10T07:05:30Z | |
dc.date.issued | 2020 | |
dc.description.abstract | We present infrared luminosity functions and dust mass functions for the EAGLE cosmological simulation, based on synthetic multiwavelength observations generated with the SKIRT radiative transfer code. In the local Universe, we reproduce the observed infrared luminosity and dust mass functions very well. Some minor discrepancies are encountered, mainly in the high luminosity regime, where the EAGLE-SKIRT luminosity functions mildly but systematically underestimate the observed ones. | en_US |
dc.identifier.citation | Marchetti, L. et al. (2020). Infrared luminosity functions and dust mass functions in the EAGLE simulation. Monthly Notices of the Royal Astronomical Society, 494(2), 2912–2924 | en_US |
dc.identifier.issn | 1365-2966 | |
dc.identifier.uri | http://hdl.handle.net/10566/5881 | |
dc.language.iso | en | en_US |
dc.publisher | Oxford University Press | en_US |
dc.subject | Hydrodynamics | en_US |
dc.subject | Radiative transfer | en_US |
dc.subject | Galaxies: evolution | en_US |
dc.subject | Cosmology: observations | en_US |
dc.title | Infrared luminosity functions and dust mass functions in the EAGLE simulation | en_US |
dc.type | Article | en_US |