2019Proceedings of the International Astronomical UnionOpen access

A full pipeline for modelling low surface brightness galaxies

Marius Peper, Boudewijn F. Roukema, Krzysztof Bolejko

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Abstract

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.

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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.

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Available abstract

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.

Key concepts: Surface brightness, Dark matter, Pipeline (software), Galaxy, Galaxy formation and evolution, Physics, Astrophysics, Halo

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