Measuring an annual modulation in a direct Dark Matter detection experiment
is not only a proof of the existence of WIMPs but can also tell us more about
their interaction with standard matter and maybe even their density and
velocity in the halo. Such a modulation has been measured by the DAMA/LIBRA
experiment in NaI(Tl) crystals. However, the interpretation as WIMP signal is
controversial due to contradicting results by other experiments. The SABRE
experiment aims to shed light on this controversy by detecting the annual
modulation in the same target material as DAMA with twin detectors at LNGS in
Italy and at SUPL in Australia. The two locations in the northern and southern
hemisphere allow to verify if other seasonal effects or the site have an
influence on the measurement, thus reducing systematic effects. This paper will
give an overview on the experimental design, the current status of the proof of
principle phase mainly devoted to high-purity crystal growing, and an outlook
on future plans.