The Astronomical Journal (Jan 2023)

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

  • 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

DOI
https://doi.org/10.3847/1538-3881/acdac7
Journal volume & issue
Vol. 166, no. 1
p. 30

Abstract

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We confirm the planetary nature of two gas giants discovered by TESS to transit M dwarfs with stellar companions at wide separations. TOI-3984 A ( J = 11.93) is an M4 dwarf hosting a short-period (4.353326 ± 0.000005 days) gas giant ( M _p = 0.14 ± 0.03 M _J and R _p = 0.71 ± 0.02 R _J ) with a wide-separation white dwarf companion. TOI-5293 A ( J = 12.47) is an M3 dwarf hosting a short-period (2.930289 ± 0.000004 days) gas giant ( M _p = 0.54 ± 0.07 M _J and R _p = 1.06 ± 0.04 R _J ) with a wide-separation M dwarf companion. We characterize both systems using a combination of ground- and space-based photometry, speckle imaging, and high-precision radial velocities from the Habitable-zone Planet Finder and NEID spectrographs. TOI-3984 A b ( T _eq = 563 ± 15 K and $\mathrm{TSM}={138}_{-27}^{+29}$ ) and TOI-5293 A b ( ${T}_{\mathrm{eq}}={675}_{-30}^{+42}$ K and TSM = 92 ± 14) are two of the coolest gas giants among the population of hot Jupiter–sized gas planets orbiting M dwarfs and are favorable targets for atmospheric characterization of temperate gas giants and 3D obliquity measurements to probe system architecture and migration scenarios.

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