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Simulations of the galaxy population constrained by observations from z=3 to the present day: implications for galactic winds and the fate of their ejecta
journal contribution
posted on 2023-06-08, 15:02 authored by Bruno M B Henriques, Simon D M White, Peter ThomasPeter Thomas, Raul E Angulo, Qi Guo, Gerard Lemson, Volker SpringelWe apply Monte Carlo Markov Chain (MCMC) methods to large-scale simulations of galaxy formation in a LambdaCDM cosmology in order to explore how star formation and feedback are constrained by the observed luminosity and stellar mass functions of galaxies. We build models jointly on the Millennium and Millennium-II simulations, applying fast sampling techniques which allow observed galaxy abundances over the ranges 7
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Publication status
- Published
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- Published version
Journal
Monthly Notices of the Royal Astronomical SocietyISSN
0035-8711Publisher
Wiley-BlackwellExternal DOI
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4Volume
431Page range
3373-3395Department affiliated with
- Physics and Astronomy Publications
Full text available
- Yes
Peer reviewed?
- Yes
Legacy Posted Date
2013-05-23First Open Access (FOA) Date
2013-05-23First Compliant Deposit (FCD) Date
2013-05-23Usage metrics
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