Galaxy formation spanning cosmic history

@article{Benson2010GalaxyFS,
  title={Galaxy formation spanning cosmic history},
  author={Andrew J. Benson and Richard G. Bower California Institute of Technology and University of Durham},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={405},
  pages={1573-1623}
}
Over the past several decades, galaxy formation theory has met with significant successes. In order to test current theories thoroughly we require predictions for as yet unprobed regimes. To this end, we describe a new implementation of the Galform semi-analytic model of galaxy formation. Our motivation is the success of the model described by Bower et al. in explaining many aspects of galaxy formation. Despite this success, the Bower et al. model fails to match some observational constraints… Expand
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References

SHOWING 1-10 OF 190 REFERENCES
The Epoch of Galaxy Formation
We use a semianalytic model of galaxy formation in hierarchical clustering theories to interpret recent data on galaxy formation and evolution, focusing primarily on the recently discoveredExpand
Galaxy morphology in the ΛCDM cosmology
We investigate the origins of galaxy morphology (defined by bulge-to-total K-band luminosity) in the A cold dark matter (ACDM) cosmology using two galaxy formation models based on the MillenniumExpand
galics– III. Properties of Lyman-break galaxies at a redshift of 3
This paper illustrates how mock observational samples of high-redshift galaxies with sophisticated selection criteria can be extracted from the predictions of GALICS, a hybrid model of hierarchicalExpand
Galaxy evolution in the infrared: comparison of a hierarchical galaxy formation model with Spitzer data
We present predictions for the evolution of the galaxy luminosity function, number counts and redshift distributions in the IR based on theCDM cosmological model. We use the combined GALFORMExpand
Semi-analytic modelling of galaxy formation: The local Universe
Using semi-analytic models of galaxy formation, we investigate galaxy properties such as the Tully-Fisher relation, the B and K-band luminosity functions, cold gas contents, sizes, metallicities, andExpand
A recipe for galaxy formation
We present a detailed prescription for how galaxy formation can be modelled in hierarchical theories of structure formation. Our model incorporates the formation and merging of dark matter halos, theExpand
Breaking the hierarchy of galaxy formation
Recent observations of the distant Universe suggest that much of the stellar mass of bright galaxies was already in place at z > 1. This presents a challenge for models of galaxy formation becauseExpand
On the Normalization of the Cosmic Star Formation History
Strong constraints on the cosmic star formation history (SFH) have recently been established using ultraviolet and far-infrared measurements, refining the results of numerous measurements over theExpand
Hybrid galaxy evolution modelling: Monte Carlo Markov Chain parameter estimation in semi-analytic models of galaxy formation
We introduce a statistical exploration of the parameter space of the Munich semi-analytic model built upon the Millennium dark matter simulation. This is achieved by applying a Monte Carlo MarkovExpand
Hierarchical galaxy formation
We describe the GALFORM semi-analytic model for calculating the formation and evolution of galaxies in hierarchical clustering cosmologies. It improves upon, and extends, the earlier scheme developedExpand
...
1
2
3
4
5
...