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Optical depth in polarised Monte Carlo radiative transfer
Maarten Baes, Christian Peest, Peter Camps +1
Context: The Monte Carlo method is the most widely used method to solve radiative transfer problems in astronomy, especially in a fully general 3D geometry. A crucial concept in an…
An evolving and mass dependent - relation for galaxies
Antonios Katsianis, Xianzhong Zheng, Valentino Gonzalez +10
The scatter () of the specific star formation rates (sSFRs) of galaxies is a measure of the diversity in their star formation histories (SFHs) at a given mass…
The cosmic spectral energy distribution in the EAGLE simulation
Maarten Baes, Ana Trčka, Peter Camps +4
The cosmic spectral energy distribution (CSED) is the total emissivity as a function of wavelength of galaxies in a given cosmic volume. We compare the observed CSED from the UV to…
The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation
Stuart McAlpine, Ian Smail, Richard G. Bower +7
We exploit EAGLE, a cosmological hydrodynamical simulation, to reproduce the selection of the observed sub-millimeter (submm) galaxy population by selecting the model galaxies at $…