Infrared luminosity functions and dust mass functions in the EAGLE simulation

dc.contributor.authorMarchetti, Lucia
dc.contributor.authorBaes, Maarten
dc.contributor.authorTrcka, Ana
dc.date.accessioned2021-02-10T07:05:30Z
dc.date.available2021-02-10T07:05:30Z
dc.date.issued2020
dc.description.abstractWe 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.citationMarchetti, L. et al. (2020). Infrared luminosity functions and dust mass functions in the EAGLE simulation. Monthly Notices of the Royal Astronomical Society, 494(2), 2912–2924en_US
dc.identifier.issn1365-2966
dc.identifier.urihttp://hdl.handle.net/10566/5881
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectHydrodynamicsen_US
dc.subjectRadiative transferen_US
dc.subjectGalaxies: evolutionen_US
dc.subjectCosmology: observationsen_US
dc.titleInfrared luminosity functions and dust mass functions in the EAGLE simulationen_US
dc.typeArticleen_US

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