All Outputs (3)

Data Release of UV to Submillimeter Broadband Fluxes for Simulated Galaxies from the EAGLE Project (2018)
Journal Article
Camps, P., Trc̆ka, A., Trayford, J., Baes, M., Theuns, T., Crain, R. A., …Schaye, J. (2018). Data Release of UV to Submillimeter Broadband Fluxes for Simulated Galaxies from the EAGLE Project. Astrophysical Journal Supplement, 234(2), Article 20. https://doi.org/10.3847/1538-4365/aaa24c

We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE suite of cosmological hydrodynamical simulations, calculated with the SKIRT radiative transfer code. The post-processing procedure includes specific c... Read More about Data Release of UV to Submillimeter Broadband Fluxes for Simulated Galaxies from the EAGLE Project.

Quantifying the impact of mergers on the angular momentum of simulated galaxies (2017)
Journal Article
Lagos, C. D. P., Stevens, A., Bower, R., Davis, T., Contreras, S., Padilla, N., …Theuns, T. (2018). Quantifying the impact of mergers on the angular momentum of simulated galaxies. Monthly Notices of the Royal Astronomical Society, 473(4), 4956-4974. https://doi.org/10.1093/mnras/stx2667

We use EAGLE to quantify the effect galaxy mergers have on the stellar specific angular momentum of galaxies, jstars. We split mergers into dry (gas-poor)/wet (gas-rich), major/minor and different spin alignments and orbital parameters. Wet (dry) mer... Read More about Quantifying the impact of mergers on the angular momentum of simulated galaxies.

Small-scale galaxy clustering in the eagle simulation (2017)
Journal Article
Artale, M. C., Pedrosa, S. E., Trayford, J. W., Theuns, T., Farrow, D. J., Norberg, P., …Schaller, M. (2017). Small-scale galaxy clustering in the eagle simulation. Monthly Notices of the Royal Astronomical Society, 470(2), 1771-1787. https://doi.org/10.1093/mnras/stx1263

We study present-day galaxy clustering in the EAGLE cosmological hydrodynamical simulation. EAGLE’s galaxy formation parameters were calibrated to reproduce the redshift z = 0.1 galaxy stellar mass function, and the simulation also reproduces galaxy... Read More about Small-scale galaxy clustering in the eagle simulation.