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Weywot, an Unusually Low-albedo Satellite in the Trans-Neptunian Region

  • Authors: Estela Fernández-Valenzuela, Bryan J. Holler, Jose Luis Ortiz, Flavia Luane Rommel, Benjamin Proudfoot, Cameron Collyer, Mónica Vara-Lubiano, Nicolas Morales, Rodrigo Leiva, Marc W. Buie, Stephen E. Levine, Michael Collins, Vadim Nikitin, Michael F. Skrutskie, Anne J. Verbiscer, Wayne Rosing, Bruno Morgado, Altair Ramos Gomes Júnior, Mike Kretlow, Josselin Desmars, Chrystian Luciano Pereira, Xavier Inosencio, Pablo Santos-Sanz, Yücel Kiliç, John Stansberry, Rosemary Pike, Amanda A. Sickafoose, Carlos A. Zuluaga, Amanda S. Bosh, Michael J. Person, Karsten Schindler, Robert Jones, Riley DeColibus, Joel H. Castro-Chacón, Nancy Chanover, Russet McMillan, Richard Boyle, Aaron Golden, Michael Ryan, Ryder Strauss, Hannah Zigo, Simon Porter, Malia Kao

Estela Fernández-Valenzuela et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 5.

Corner plot showing the posterior distribution from our MCMC ellipse fit, including the RECON24 chord. At the top of each column are the marginal (one-dimensional) posterior distributions for each parameter; beneath those, joint (two-dimensional) posterior distributions are shown for each pair of parameters. Contours show the 0.5σ, 1σ, 1.5σ, and 2σ confidence regions. Black points correspond to samples from the MCMC chain.

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