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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Julien Devriendt

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Cosmology
  • Galaxy formation and evolution
julien.devriendt@physics.ox.ac.uk
Telephone: 01865 (2)73307
Denys Wilkinson Building, room 555D
  • About
  • Teaching
  • Publications

GALICS - I. A hybrid N-body/semi-analytic model of hierarchical galaxy formation

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 343:1 (2003) 75-106

Authors:

S Hatton, JEG Devriendt, S Ninin, FR Bouchet, B Guiderdoni, D Vibert

GALICS: A Direct Link between Theory and Observations

Chapter in The Evolution of Galaxies, Springer Nature (2003) 75-78

Non-Standard Structure Formation Scenarios

Chapter in The Evolution of Galaxies, Springer Nature (2003) 41-46

Authors:

Alexander Knebe, Brett Little, Ranty Islam, Julien Devriendt, Asim Mahmood, Joe Silk

Predicting Multi-Wavelength Properties of Lyman Break Galaxies with GalICS

Chapter in The Evolution of Galaxies, Springer Nature (2003) 79-82

Authors:

J茅r茅my Blaizot, Bruno Guiderdoni, Julien EG Devriendt, Francqis R Bouchet, Steve Hatton

Predicting multi-wavelength properties of Lyman break galaxies with GalICS

ASTROPHYS SPACE SCI 284:2 (2003) 373-376

Authors:

J Blaizot, B Guiderdoni, JEG Devriendt, FR Bouchet, S Hatton

Abstract:

GalICS (for GALaxies In Cosmological Simulations) is a model of hierarchical galaxy formation which combines high resolution numerical simulations for the dark matter component with semi-analytic prescriptions for the baryonic matter. It provides us with an explicit cosmological framework to analyse observations of distant galaxies, and to understand how they evolve to become local galaxies. We use GalICS to build multi-wavelength mock galaxy catalogues which include clustering properties. We can compare them to the sample of Lyman Break Galaxies at z=3 ( Steidel et al., 1996), and to deep sub-mm surveys. The predictions of the model will be detailed, and show a good agreement with the available data.

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