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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 7.

TSM, as defined in Kempton et al. (2018), for TOIs in multiplanet systems around bright M dwarfs (T eff < 4000 K and T mag < 11.5) with R p < 4 R ⊕ as of 2022 July 7. TIC stars are sorted in decreasing order of second largest TSM value in the system. Color corresponds to host T mag and size corresponds to planet radius. The gray dashed line is the atmospheric follow-up threshold recommended by Guerrero et al. (2021) for sub-Neptunes. TOI 4342 is among the top 10 systems with multiple planets that are well suited for atmospheric characterization.

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