Figure 3 from Detection and Bulk Properties of the HR 8799 Planets with High-resolution Spectroscopy

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Detection and Bulk Properties of the HR 8799 Planets with High-resolution Spectroscopy

Authors: Jason J. Wang, Jean-Baptiste Ruffio, Evan Morris, Jacques-Robert Delorme, Nemanja Jovanovic, Jacklyn Pezzato, Daniel Echeverri, Luke Finnerty, Callie Hood, J. J. Zanazzi, Marta L. Bryan, Charlotte Z. Bond, Sylvain Cetre, Emily C. Martin, Dimitri Mawet, Andy Skemer, Ashley Baker, Jerry W. Xuan, J. Kent Wallace, Ji Wang, Randall Bartos, Geoffrey A. Blake, Andy Boden, Cam Buzard, Benjamin Calvin, Mark Chun, Greg Doppmann, Trent J. Dupuy, Gaspard Duchêne, Y. Katherina Feng, Michael P. Fitzgerald, Jonathan Fortney, Richard S. Freedman, Heather Knutson, Quinn Konopacky, Scott Lilley, Michael C. Liu, Ronald Lopez, Roxana Lupu, Mark S. Marley, Tiffany Meshkat, Brittany Miles, Maxwell Millar-Blanchaer, Sam Ragland, Arpita Roy, Garreth Ruane, Ben Sappey, Tobias Schofield, Lauren Weiss, Edward Wetherell, Peter Wizinowich, and Marie Ygouf

2021 The Astronomical Journal 162 148.

Provider: AAS Journals

Caption: Figure 3.

Posterior distributions of the main planetary parameters for each planet in the Full Model fit. In the bottom-left panel, the gray shaded region represents the 68% credible interval of the radial velocity of the host star relative to the solar system barycenter.

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