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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 detection detections of flare stars.
- Blind survey transient detections and ultrain both the image-plane and VCS data.
- Ultra-long period transients.
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