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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 3.

Light curves from all sites relative to the predicted time. The predicted time is indicated in dotted–dashed green vertical lines, the 1σ in dashed green and 2σ in solid green. Flux is normalized to unity when the star is not occulted. The right side shows the site code and name, cross-track predicted distance, and predicted time in UTC. An electronic copy of the data in this figure is provided. In red we highlight all data points higher or lower than 2σ, using the average S/N from each light curve. The labels 1, 2, and 3 identify the three groups of consecutive flux drops which are possible detections.

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

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