A full pipeline for modelling low surface brightness galaxies

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Cambridge University Press

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.

Description

Accepted 17.09.2019. In press

Keywords

methods: numerical, galaxies: evolution, cosmology: dark matter

Citation

IAUS353

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