The young massive SMC cluster NGC 330 seen by MUSE - II. Multiplicity properties of the massive-star population

The authors acknowledge support from the FWO_Odysseus program under project G0F8H6N and from the European Space Agency (ESA) and the Belgian Federal Science Policy Office (BELSPO) through the PRODEX Programme. The research leading to these results has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement numbers 772225: MULTIPLES). Parts of the analysis in this project are based on the python code photutils.