ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …

The relation between halo mass, M, and concentration, c, is a critical component in our
understanding of the structure of dark matter halos. While numerous models for this relation …

Galaxies fall into two clearly distinct types:'blue-sequence'galaxies that are rapidly forming
young stars, and 'red-sequence'galaxies in which star formation has almost completely …

We use a suite of cosmological simulations to study the mass–concentration–redshift
relation, c (M, z), of dark matter haloes. Our simulations include standard Λ-cold dark matter …

We investigate the internal structure and density profiles of haloes of mass 1010–1014 M⊙
in the Evolution and Assembly of Galaxies and their Environment (EAGLE) simulations …

The observed anticorrelation between the central dark matter (DM) densities of the bright
Milky Way (MW) dwarf spheroidal galaxies (dSphs) and their orbital pericentre distances …

We present a semi-analytic, physically motivated model for dark matter halo concentration
as a function of halo mass and redshift. The semi-analytic model combines an analytic …

ABSTRACT Recent Atacama Large Millimeter Array large surveys unveiled the presence of
significant dust continuum emission in star-forming galaxies at z> 4. Unfortunately, such …

We present 25 cosmological zoom-in simulations of Milky-Way-mass galaxies in the
'MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE'(E …

We use the hydrodynamical EAGLE simulation to study the magnitude and origin of the
scatter in the stellar mass-halo mass relation for central galaxies. We separate cause and …