Fig. 1.
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Posterior distributions of IMBH orbits. Left: posterior distribution over the mass and semi-major axis of the IMBH for orbits with a semi-major axis smaller than 0.1″. The contours correspond to 39%, 86%, and 98.8% (from dark blue to light blue) enclosed likelihood. Right: same as left, but for orbits extending out to a semi-major axis of 1″.
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