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First Astrometric Limits on Binary Planets and Exomoons Orbiting β Pictoris b

Authors: Isabella Macias, Sydney A. Jenkins, Andrew Vanderburg

Isabella Macias et al 2026 The Astronomical Journal 171 .

Provider: AAS Journals

Caption: Figure 2.

Predicted separation of both β Pic b and c in our best-fit “two-planet“ model (solid gray curves), along with the actual observed separations. The dark purple points represent GRAVITY observations, while the lighter purple points represent SPHERE observations.

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