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TOI-3984 A b and TOI-5293 A b: Two Temperate Gas Giants Transiting Mid-M Dwarfs in Wide Binary Systems

Authors: Caleb I. Cañas, Shubham Kanodia, Jessica Libby-Roberts, Andrea S. J. Lin, Maria Schutte, Luke Powers, Sinclaire Jones, Andrew Monson, Songhu Wang, Guđmundur Stefánsson, William D. Cochran, Paul Robertson, Suvrath Mahadevan, Adam F. Kowalski, John Wisniewski, Brock A. Parker, Alexander Larsen, Franklin A. L. Chapman, Henry A. Kobulnicky, Arvind F. Gupta, Mark E. Everett, Bryan Edward Penprase, Gregory Zeimann, Corey Beard, Chad F. Bender, Knicole D. Colón, Scott A. Diddams, Connor Fredrick, Samuel Halverson, Joe P. Ninan, Lawrence W. Ramsey, Arpita Roy, Christian Schwab

Caleb I. Cañas et al 2023 The Astronomical Journal 166 .

Provider: AAS Journals

Caption: Figure 4.

Same as Figure 3 but for TOI-5293 A. (a) Median normalized TESS light curve for TOI-5293 A derived with eleanor along with the best-fitting Gaussian process model. The triangles indicate the observed transits. Panels (b)−(g) are the light curves for the TESS, RBO, LCRO, and TMMT plotted with model posteriors (shaded regions) from the joint fit to the photometry and RVs.

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