Aims. Understanding the link between the galaxy properties and the dark matter halos they
reside in and their coevolution is a powerful tool for constraining the processes related to …

In this work, we combine the semi-analytic model of galaxy formation and evolution sag with
the 102 relaxed simulated galaxy clusters from the three hundred project, and we study the …

Reproducing the observed quenched fraction of satellite galaxies has been a long-standing
issue for galaxy formation models. We modify the treatment of environmental effects in our …

Background The use of liquid biopsy is of potential high importance for children with high
grade (HGG) and diffuse midline gliomas (DMG), particularly where surgical procedures are …

We use the Evolution and Assembly of GaLaxies and their Environments (EAGLE)
hydrodynamical simulation to trace the quenching history of galaxies in its 10 most massive …

We analyse the connection between the star formation quenching of galaxies and their
location in the outskirts of clusters in the redshift range z=[0, 2] by estimating the fraction of …

We explore the build-up of quiescent galaxies using a sample of 28 469 massive (M⋆≥
1011 M⊙) galaxies at redshifts 1.5<< 3.0, drawn from a 17.5 deg2 area (0.33 Gpc3 …

Hydrodynamic simulations provide a powerful, but computationally expensive, approach to
study the interplay of dark matter and baryons in cosmological structure formation. Here, we …

We study environmental quenching using the spatial distribution of current star formation
and stellar population ages with the full SAMI Galaxy Survey. By using a star formation …

The current properties of globular cluster systems (GCSs) are the result of the evolution
experienced by their host galaxies, which shape the richness of the GCS as well as its …