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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

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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 Springel
We 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

History

Publication status

  • Published

File Version

  • Published version

Journal

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

Publisher

Wiley-Blackwell

Issue

4

Volume

431

Page range

3373-3395

Department affiliated with

  • Physics and Astronomy Publications

Full text available

  • Yes

Peer reviewed?

  • Yes

Legacy Posted Date

2013-05-23

First Open Access (FOA) Date

2013-05-23

First Compliant Deposit (FCD) Date

2013-05-23

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