Figure 3 from Non-detection of Contamination by Stellar Activity in the Spitzer Transit Light Curves of TRAPPIST-1

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Non-detection of Contamination by Stellar Activity in the Spitzer Transit Light Curves of TRAPPIST-1

Authors: Brett M. Morris, Eric Agol, Leslie Hebb, Suzanne L. Hawley, Michaël Gillon, Elsa Ducrot, Laetitia Delrez, James Ingalls, and Brice-Olivier Demory

2018 The Astrophysical Journal Letters 863 L32.

Provider: AAS Journals

Caption: Figure 3.

Posterior distributions for p₀ and p₁ for planets b through h. All of the planets present p₀ ≈ p₁, suggesting that the photospheric intensity within transit chords of the planets is roughly representative of the rest of the stellar photosphere.

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