Figure 1 from New Insights on Planet Formation in WASP-47 from a Simultaneous Analysis of Radial Velocities and Transit Timing Variations

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New Insights on Planet Formation in WASP-47 from a Simultaneous Analysis of Radial Velocities and Transit Timing Variations

Authors: Lauren M. Weiss, Katherine M. Deck, Evan Sinukoff, Erik A. Petigura, Eric Agol, Eve J. Lee, Juliette C. Becker, Andrew W. Howard, Howard Isaacson, Ian J. M. Crossfield, Benjamin J. Fulton, Lea Hirsch, and Björn Benneke

2017 The Astronomical Journal 153 265.

Provider: AAS Journals

Caption: Figure 1.

Observed minus linear-ephemeris calculated transit times of WASP-47 e (blue points, top panel), b (green points, middle panel), and d (brown points, bottom panel). The best-fit N-body model to the TTVs alone (using TTVFast, black connected dots) and the best-fit analytic model to the TTVs alone (using TTVFaster, gray connected dots) are shown.

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