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The True Stellar Obliquity of a Sub-Saturn Planet from the Tierras Observatory and the Keck Planet Finder

  • Authors: Patrick Tamburo, Samuel W. Yee, Juliana García-Mejía, Gudmundur Stefánsson, David Charbonneau, Allyson Bieryla, Andrew W. Howard, Howard Isaacson, Benjamin J. Fulton, Aaron Householder

Patrick Tamburo et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Top: Tierras light curve of TOI-2364. Data at the native 30 s cadence are shown in gray, with their error bars scaled by a factor of 1.66 compared to our calculated photometric uncertainties. White points points with error bars show the median flux measured on each night. The best-fit QP-GP model is shown as a green line, along with its 1 and 2σ uncertainty intervals as shaded regions. Bottom: the residuals from the best-fit QP-GP model.

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