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Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
Anna de Graaff, James Trayford, Marijn Franx +3
We use mock images of galaxies in the 100 Mpc EAGLE simulation to establish the differences between the sizes and morphologies inferred from the stellar mass distributions…
SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
Sampath Mukherjee, Léon V. E. Koopmans, Crescenzo Tortora +4
The central dark-matter fraction of galaxies is sensitive to feedback processes during galaxy formation. Strong gravitational lensing has been effective in the precise measurement…
The importance of black hole repositioning for galaxy formation simulations
Yannick M. Bahé, Joop Schaye, Matthieu Schaller +6
Active galactic nucleus (AGN) feedback from accreting supermassive black holes (SMBHs) is an essential ingredient of galaxy formation simulations. The orbital evolution of SMBHs is…
A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
Christopher C. Lovell, Stephen M. Wilkins, Peter A. Thomas +4
High-resolution cosmological hydrodynamic simulations are currently limited to relatively small volumes due to their computational expense. However, much larger volumes are require…
A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
M. Icaza-Lizaola, Richard G. Bower, Peder Norberg +3
Sparse regression algorithms have been proposed as the appropriate framework to model the governing equations of a system from data, without needing prior knowledge of the underlyi…