From particles to pixels: how many particles do I really need to construct stellar kinematic mock observational measurements?
This work considers the impact of resolution in the construction of mock observations of simulated galaxies. In particular, when building mock integral field spectroscopic observations from galaxy formation models in cosmological simulations, we investigate the possible systematics that may arise gi...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2024-11, Vol.535 (3), p.2844-2862 |
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Hauptverfasser: | , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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