A full pipeline for modelling low surface brightness galaxies

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dc.contributor.authorPeper, Marius
dc.contributor.authorRoukema, Boudewijn
dc.contributor.authorBolejko, Krzysztof
dc.contributor.supervisorRoukema, Boudewijn
dc.date.accessioned2020-02-01T14:46:22Z
dc.date.available2020-02-01T14:46:22Z
dc.date.issued2019-09-07
dc.descriptionAccepted 17.09.2019. In presspl
dc.description.abstractCosmological 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.pl
dc.description.sponsorshipInstitute of Astronomy NCUpl
dc.identifier.citationIAUS353pl
dc.identifier.issn1743-9221
dc.identifier.urihttp://repozytorium.umk.pl/handle/item/6239
dc.language.isoengpl
dc.publisherCambridge University Presspl
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectmethods: numericalpl
dc.subjectgalaxies: evolutionpl
dc.subjectcosmology: dark matterpl
dc.titleA full pipeline for modelling low surface brightness galaxiespl
dc.typeinfo:eu-repo/semantics/preprintpl
dc.typeinfo:eu-repo/semantics/conferenceObjectpl

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