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Stellar Occultation by the Resonant Trans-Neptunian Object (523764) 2014 WC510 Reveals a Close Binary TNO

  • Authors: Rodrigo Leiva, Marc W. Buie, John M. Keller, Lawrence H. Wasserman, JJ Kavelaars, Terry Bridges, Sean L. Haley, Ryder Strauss, Elizabeth Wilde, Robert Weryk, Pierre Kervella, Robert Baker, Stephen Alan Bock, Ken Conway, Juan M. Cota, James J. Estes, María L. García, Matthew Kehrli, Andrew McCandless, Keitha McCandless, Edgar Self, Cole Settlemire, Diana J. Swanson, Doug Thompson, and J.A. Wise

2020 The Planetary Science Journal 1 48.

  • Provider: AAS Journals

Caption: Figure 7.

Posterior pdf for the diameters and geometric albedo for the favored model ﹩{{ \mathcal M }}_{5}﹩. Diagonal panels: marginalized posterior pdf for the diameter of the primary, the secondary, and the geometric albedo. The nominal values are indicated by the dotted lines, while the dashed vertical lines are the 68% credible intervals. The three remaining panels in the bottom left are the joint posterior pdf for the same parameters. The contours in the joint pdf’s are the 39.3% credible intervals.

(The data used to create this figure are available.)

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