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TESS Discovery of Twin Planets near 2:1 Resonance around Early M Dwarf TOI 4342

Authors: Evan Tey, Chelsea X. Huang, Michelle Kunimoto, Andrew Vanderburg, Avi Shporer, Samuel N. Quinn, George Zhou, Karen A. Collins, Kevin I. Collins, Eric L. N. Jensen, Richard P. Schwarz, Ramotholo Sefako, Tianjun Gan, Elise Furlan, Crystal L. Gnilka, Steve B. Howell, Kathryn V. Lester, Carl Ziegler, César Briceño, Nicholas Law, Andrew W. Mann, George R. Ricker, Roland K. Vanderspek, David W. Latham, S. Seager, Jon M. Jenkins, Joshua N. Winn, Douglas A. Caldwell, David Charbonneau, Christopher J. Burke, Zahra Essack

Evan Tey et al 2023 The Astronomical Journal 165 .

Provider: AAS Journals

Caption: Figure 8.

Insolation and orbital period vs. planet size. TOI 4342 b and TOI 4342 c are shown in cyan over occurrence contours for host stars with M _* < 0.97 M _⊙ from Fulton & Petigura (2018). M-dwarf TOIs as of 2022 July 7 are plotted as well, with multiplanet system planets highlighted in magenta. TOI 4342 b and TOI 4342 c both lie in the upper end of the radius valley.

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