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Fig. 6


Top, flux-density ratio of the NE image to the SW image. Bottom, flux density of the NE image. Circles are the ALMA data and lines are the predictions from our best-fit jet model. Different colors correspond to different observing epochs. Left, fit to the conical-jet model. Right, fit to the concave-jet model. The dashed line marks the lower flux-density ratio expected from an (unconstrained) previous flare (see text for details).

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