Globular clusters are large and dense agglomerate of stars. At variance with smaller clusters
of stars, they exhibit signs of some chemical evolution. At least for this reason, they are …

The growing population of binary black holes (BBHs) observed by gravitational wave (GW)
detectors is a potential Rosetta stone for understanding their formation channels. Here, we …

In this paper we describe a new UV-initiative Hubble Space Telescope project (GO-13297)
that will complement the existing F606W and F814W database of the Advanced Camera for …

We utilise multi-epoch MUSE spectroscopy to study binary stars in the core of the Galactic
globular cluster NGC 3201. Our sample consists of 3553 stars with 54 883 spectra in total …

We present new constraints on the star formation histories of six ultra-faint dwarf galaxies:
Bootes I, Canes Venatici II, Coma Berenices, Hercules, Leo IV, and Ursa Major I. Our …

This is the first of a series of papers presenting the results from our survey of 25 Galactic
globular clusters with the MUSE integral-field spectrograph. In combination with our …

In this paper, we present the astrophotometric catalogues of 56 globular clusters and one
open cluster. Astrometry and photometry are mainly based on images collected within the …

Our current understanding of the stellar initial mass function and massive star evolution
suggests that young globular clusters (GCs) may have formed hundreds to thousands of …

In the past few years, we have undertaken an extensive investigation of star clusters and
their stellar populations in the Large and Small Magellanic Clouds (LMC and SMC) based …

The absolute age of a simple stellar population is of fundamental interest for a wide range of
applications but is difficult to measure in practice, as it requires an understanding of the …