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Journal article

The new semi-analytic code GalICS 2.0 – reproducing the galaxy stellar mass function and the Tully–Fisher relation simultaneously

Abstract:

GalICS 2.0 is a new semianalytic code to model the formation and evolution of galaxies in a cosmological context. N-body simulations based on a Planck cosmology are used to construct halo merger trees, track subhaloes, compute spins and measure concentrations. The accretion of gas onto galaxies and the morphological evolution of galaxies are modelled with prescriptions derived from hydrodynamic simulations. Star formation and stellar feedback are described with phenomenologi...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Accepted manuscript

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Publisher copy:
10.1093/mnras/stx1597

Authors


Cattaneo, A More by this author
Blaizot, J More by this author
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
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Publisher:
Oxford University Press (OUP) Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Issue:
2
Publication date:
2017-07-14
Acceptance date:
2017-06-22
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:702637
URN:
uri:d22bc66a-f60f-493f-8c29-7c8e9a1c8239
UUID:
uuid:d22bc66a-f60f-493f-8c29-7c8e9a1c8239
Local pid:
pubs:702637

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