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- MWA rapid-response (automated triggering) on high energy (GRBs, flare stars) and multi-messenger (GWs, FRBs, neutrinos) transients using the standard corrector and VCS.
- Stokes V detections of flaring stars and star-(exo)planet interactions.
- Blind survey transient detections (meteors, space debris, satellites) in both the image-plane and VCS data.
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