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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 10.

(a) TOI-3984 A b (star) and TOI-5293 A b (diamond star) on the mass–radius diagram for transiting M dwarf exoplanets with mass measurements and R _p > 4 R _⊕. All previously known hot Jupiters (P < 10 days and R _P ≥ 8 R _⊕) transiting M dwarfs are marked as pentagons. (b) TOI-3984 A and TOI-5293 A on an effective temperature–surface gravity diagram. (c) Insolation flux and radius for these planets. The data were compiled from the NASA Exoplanet Archive (Akeson et al. 2013) on 2023 May 3.

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