Barberio, E.Baroncelli, T.Bignell, L. J.Bolognino, I.Brooks, G.Dastgiri, F.Duffy, A. R.Froehlich, M.Fu, G.Gerathy, M. S.M.Hill, G. C.Krishnan, S.Lane, G. J.Lawrence, G.Leaver, K. T.Mahmood, I.McGee, P.McKie, L.McNamara, P. C.Mews, M.Melbourne, W. J.D.Milana, G.Milligan, L. J.Mould, J.Scutti, F.Slavkovská, Z.Spinks, N. J.Stanley, O.Stuchbery, A. E.Taylor, G. N.Urquijo, P.Williams, A. G.Zhong, Y. Y.Zurowski, M. J.2025-06-102025-06-10ORCID:/0000-0002-0198-9901/work/162367340http://www.scopus.com/inward/record.url?scp=85149945369&partnerID=8YFLogxKhttps://hdl.handle.net/1885/733757968The SABRE (Sodium iodide with Active Background REjection) experiment aims to provide a model independent test of the signal observed by DAMA/LIBRA by detecting an annual modulation from dark matter interactions in ultra-high purity NaI(Tl) crystals. SABRE consists of two detectors: SABRE North, located at the Laboratori Nazionali del Gran Sasso (LNGS), and SABRE South, located at the newly completed Stawell Underground Physics Laboratory (SUPL) in Stawell, Australia - the first deep underground laboratory in the Southern Hemisphere. Here we present the status of both the SABRE South experiment and SUPL.This work was supported by the ARC grant DP190103123, and the ARC Centre of Excellence for Dark Matter Particle Physics through grant CE200100008. This research was partially supported by Australian Government Research Training Program Scholarships, and Melbourne Research Scholarships.enPublisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)202285149945369