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.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.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.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