Fig. C.1.

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Impact of modifying parameters of the fiducial model: Keplerianity and orbital radius with a fixed orbital period (left), black hole spin (center), and inclination (right). The presence and size of the small inner loop puts strong constraints on the inclination and orbital radius admitted by the vertical magnetic field model. Additionally, in the vertical magnetic field model framework, the observed loop size may suggest a large positive spin of Sgr A*.
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