Constraining cosmology with the velocity function of low-mass galaxies
The number density of field galaxies per rotation velocity, referred to as the velocity function, is an intriguing statistical measure probing the smallest scales of structure formation. In this paper we point out that the velocity function is sensitive to small shifts in key cosmological parameters...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
10 January 2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 475, Heft: 4, Pages: 4809-4824 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty054 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/sty054 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/475/4/4809/4797165 
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| Verfasserangaben: | Aurel Schneider and Sebastian Trujillo-Gomez |
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Constraining cosmology with the velocity function of low-mass galaxies
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