Figure 4 from New Insights on Planet Formation in WASP-47 from a Simultaneous Analysis of Radial Velocities and Transit Timing Variations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 4.

The best simultaneous fit to the TTVs and RVs of the WASP-47 system, and residuals. From top to bottom, the panels show the TTVs of the transiting planets e (P = 0.79 days, blue), b (P = 4.16 days, green), and d (P = 9.0 days, brown). The best simultaneous fit to the TTVs+RVs of all four planets is shown as black connected points.

Other Images in This Article

Copyright and Terms & Conditions