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A full pipeline for modelling low surface brightness galaxies


Peper, M and Roukema, BF and Bolejko, K, A full pipeline for modelling low surface brightness galaxies, Proceedings of the International Astronomical Union, 14, (S353) pp. 279-280. ISSN 1743-9213 (2019) [Refereed Article]

Copyright Statement

Copyright International Astronomical Union 2020

DOI: doi:10.1017/S1743921319008548


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.

Item Details

Item Type:Refereed Article
Keywords:cosmic flows, power spectrum, redshift surveys, galaxy clustering, galaxies, cosmology, dark matter
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:Cosmology and extragalactic astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Bolejko, K (Dr Krzysztof Bolejko)
ID Code:148270
Year Published:2019
Deposited By:Physics
Deposited On:2021-12-15
Last Modified:2022-02-25

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