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A full pipeline for modelling low surface brightness galaxies

Published online by Cambridge University Press:  14 May 2020

Marius Peper Open the ORCID record for Marius Peper [Opens in a new window] ,
Boudewijn F. Roukema Open the ORCID record for Boudewijn F. Roukema [Opens in a new window]  and
Krzysztof Bolejko Open the ORCID record for Krzysztof Bolejko [Opens in a new window]
Marius Peper
Affiliation:
Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Grudziadzka 5, Nicolaus Copernicus University, ul. Gagarina 11, 87-100 Toruń, Poland email: marius.peper@astro.umk.pl
Boudewijn F. Roukema
Affiliation:
Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Grudziadzka 5, Nicolaus Copernicus University, ul. Gagarina 11, 87-100 Toruń, Poland email: marius.peper@astro.umk.pl
Krzysztof Bolejko
Affiliation:
School of Natural Sciences, College of Sciences and Engineering, University of Tasmania Private Bag 37, Hobart, TAS 7001, Australia
Rights & Permissions [Opens in a new window]

Abstract

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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.

Keywords

methods: numericalgalaxies: evolutioncosmology: dark matter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 279 - 280
Copyright
© International Astronomical Union 2020

References

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