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Figure 3 from The Detectability of Transit Depth Variations Due to Exoplanetary Oblateness and Spin Precession Joshua A. Carter and Joshua N. Winn 2010.

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Presentation on theme: "Figure 3 from The Detectability of Transit Depth Variations Due to Exoplanetary Oblateness and Spin Precession Joshua A. Carter and Joshua N. Winn 2010."— Presentation transcript:

1 Figure 3 from The Detectability of Transit Depth Variations Due to Exoplanetary Oblateness and Spin Precession Joshua A. Carter and Joshua N. Winn 2010 ApJ doi: / X/716/1/850 Information: Thank you for downloading this PowerPoint slide from The Astrophysical Journal. This slide was designed to be edited; you can: - Remove components (including this text box!) - Resize components - Apply a style or theme - Please remember to include the original article citation information.

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