Fig. A.1
Kinematic analysis of TOI-681 exhibiting its membership to the open star cluster NGC 2516. Black points are NGC 2516 members reported by Cantat-Gaudin et al. (2018). Gray points are randomly drawn from a cube in {α, δ, π} centered on the cluster, with side widths ± 4σ, where σ is the standard deviation of the Cantat-Gaudin et al. (2018) cluster member right ascension, declination, and parallax.
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