Corpus ID: 218570977

A flexible modelling of galaxy assembly bias.

@article{Contreras2020AFM,
  title={A flexible modelling of galaxy assembly bias.},
  author={Sergio Contreras and Ra{\'u}l E. Angulo and Matteo Zennaro},
  journal={arXiv: Astrophysics of Galaxies},
  year={2020}
}
  • Sergio Contreras, Raúl E. Angulo, Matteo Zennaro
  • Published 2020
  • Physics
  • arXiv: Astrophysics of Galaxies
  • We use the {\sc Illustris TNG300} magneto-hydrodynamic simulation, the {\sc SAGE} semi-analytical model, and the subhalo abundance matching technique (SHAM) to examine the diversity in predictions for galaxy assembly bias. We consider samples of galaxies selected according to their stellar mass or star formation rate at various redshifts. We find that all models predict an assembly bias signal of different magnitude, redshift evolution, and dependence with selection criteria and number density… CONTINUE READING

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    preprint, (arXiv:1611.00366) This paper has been typeset from a TEX/LATEX file prepared by the author

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