[PDF] Top 20 A chronicle of galaxy mass assembly in the EAGLE simulation

... the mass build-up of ...the assembly of low-mass galaxies and high- mass galaxies ...secondary galaxy reaches its maximum stel- lar mass, we determine the merger type when the ... See full document

... and Assembly of GaLaxies and their Environments’ (EAGLE; Schaye et ...The EAGLE suite comprises a number of cosmological simulations performed at a range of numerical resolution, in peri- odic ... See full document

... which EAGLE galaxies move onto the red sequence depends on their mor- phological ...of EAGLE galaxies starts to build-up around z=1, due to the quenching of low-mass satellite galaxies at the faint ... See full document

... There has long been a discrepancy between the measured number density of low-luminosity galaxies (the ‘faint end’ of the LF) and predictions from cold dark matter (CDM) hierarchical sim- ulations, in the sense that fewer ... See full document

... mock galaxy catalogue, constructed from the Millennium DM simulation (Springel et ...semi-analytic galaxy formation recipe. The galaxy positions are interpolated between the Millennium ... See full document

... Due to a number of reasons, not all the galaxies that met the selection criteria described in section 3.1 also pass the requirements detailed in Appendix A2. The majority of lens candidates are not relaxed, isolated ... See full document

... A simple diagnostic of the state of the gas in a simulation is the dis- tribution of the SPH particles or grid cells in the density-temperature plane. The different components (ISM, IGM, etc.) can then be iden- ... See full document

... Lower mass galaxies (both star forming and passive) contain younger and lower metallicity stellar populations, and are there- fore bluer in colour ...primary galaxy at higher ve- locities, as both the total ... See full document

... of mass in each simulation that is part of a resolved halo: F(> m min |t) , where m min = 3 ...minimum mass is a consequence of the numerical resolution of the simulations, but is consistent ... See full document

... the galaxy size distribution as well as many other aspects of galaxy phenomenology (Furlong et ...the EAGLE simulation and its ancestor ...in EAGLE, and Sales et al. (2012) reported ... See full document

... the EAGLE relations represent the 16th to 84th percentile range, which should be comparable to the ±1 σ range provided for the ob- servational data, assuming near ...the EAGLE trend is typically larger than ... See full document

... and galaxy velocity bias induced by ignoring baryons and their back-reaction on to the DM and galaxy velocity ...the EAGLE run, we find its unique counterpart in the DMO run by identifying the ... See full document

... An alternative approach is to study voids, which contain an uncharacteristically few num- ber of galaxies. As well as being tremendously useful for the AP test, studies of voids have also provided a lower constraint for ... See full document

... Large galaxy surveys have also been a driving force in the field of galaxy evolution, although for a different ...on galaxy scales is less mature. The enormous range of mass and time-scales ... See full document

... stellar mass-sensitive K−band profiles of red and green galaxy populations are very similar, while g−band profiles indicate more disk-like morphologies for the green galaxies: apparent (optical) ... See full document

... further blocks in the South Galactic Pole). Amongst other legacy goals, the survey team will create a complete, magnitude-limited sample of galaxies with redshift and colour information from the far-ultraviolet (FUV) to ... See full document

... grain assembly in a shear box under the condition of no externally applied load was investigated numerically using the Discrete Element ...The assembly was a monodisperse system compri- sing 3000 circular ... See full document

... using EAGLE, and its dependence on the average dust surface density, Σ dust ...Ref100 EAGLE galaxies, with error bars indicating the 16-84 percentile ...contributing galaxy are ... See full document

... Large galaxy surveys have also been a driving force in the field of galaxy evolution, although for a different ...on galaxy scales is less mature. The enormous range of mass and time-scales ... See full document

... Whilst the large cluster may be missing more objects in total, its dynamics will already be reliably measurable at 80% completeness. The more tenuous small groups require very high levels of completeness to confidently ... See full document