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A full pipeline for modelling low surface brightness galaxies

Repozytorium Uniwersytetu Mikołaja Kopernika

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dc.contributor.author Peper, Marius
dc.contributor.author Roukema, Boudewijn
dc.contributor.author Bolejko, Krzysztof
dc.date.accessioned 2020-02-01T14:46:22Z
dc.date.available 2020-02-01T14:46:22Z
dc.date.issued 2019-09-07
dc.identifier.citation IAUS353
dc.identifier.issn 1743-9221
dc.identifier.uri http://repozytorium.umk.pl/handle/item/6239
dc.description Accepted 17.09.2019. In press
dc.description.abstract Cosmological simulations are a powerful tool to test various cosmological and galaxy formation scenarios. The discovery of low surface brightness objects has been a challenge for both of these fields. Our work aims to create a fully reproducible pipeline to generate a realistic dark matter halo catalog with corresponding information on galaxy formation and evolution.
dc.description.sponsorship Institute of Astronomy NCU
dc.language.iso eng
dc.publisher Cambridge University Press
dc.rights info:eu-repo/semantics/openAccess
dc.subject methods: numerical
dc.subject galaxies: evolution
dc.subject cosmology: dark matter
dc.title A full pipeline for modelling low surface brightness galaxies
dc.type info:eu-repo/semantics/preprint
dc.type info:eu-repo/semantics/conferenceObject
dc.contributor.supervisor Roukema, Boudewijn


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