The Astronomical Journal (Jan 2023)

TOI-199 b: A Well-characterized 100 day Transiting Warm Giant Planet with TTVs Seen from Antarctica

  • Melissa J. Hobson,
  • Trifon Trifonov,
  • Thomas Henning,
  • Andrés Jordán,
  • Felipe Rojas,
  • Nestor Espinoza,
  • Rafael Brahm,
  • Jan Eberhardt,
  • Matías I. Jones,
  • Djamel Mekarnia,
  • Diana Kossakowski,
  • Martin Schlecker,
  • Marcelo Tala Pinto,
  • Pascal José Torres Miranda,
  • Lyu Abe,
  • Khalid Barkaoui,
  • Philippe Bendjoya,
  • François Bouchy,
  • Marco Buttu,
  • Ilaria Carleo,
  • Karen A. Collins,
  • Knicole D. Colón,
  • Nicolas Crouzet,
  • Diana Dragomir,
  • Georgina Dransfield,
  • Thomas Gasparetto,
  • Robert F. Goeke,
  • Tristan Guillot,
  • Maximilian N. Günther,
  • Saburo Howard,
  • Jon M. Jenkins,
  • Judith Korth,
  • David W. Latham,
  • Monika Lendl,
  • Jack J. Lissauer,
  • Christopher R. Mann,
  • Ismael Mireles,
  • George R. Ricker,
  • Sophie Saesen,
  • Richard P. Schwarz,
  • S. Seager,
  • Ramotholo Sefako,
  • Avi Shporer,
  • Chris Stockdale,
  • Olga Suarez,
  • Thiam-Guan Tan,
  • Amaury H. M. J. Triaud,
  • Solène Ulmer-Moll,
  • Roland Vanderspek,
  • Joshua N. Winn,
  • Bill Wohler,
  • George Zhou

DOI
https://doi.org/10.3847/1538-3881/acfc1d
Journal volume & issue
Vol. 166, no. 5
p. 201

Abstract

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We present the spectroscopic confirmation and precise mass measurement of the warm giant planet TOI-199 b. This planet was first identified in TESS photometry and confirmed using ground-based photometry from ASTEP in Antarctica including a full 6.5 hr long transit, PEST, Hazelwood, and LCO; space photometry from NEOSSat; and radial velocities (RVs) from FEROS, HARPS, CORALIE, and CHIRON. Orbiting a late G-type star, TOI-199 b has a ${104.854}_{-0.002}^{+0.001}\,{\rm{day}}$ period, a mass of 0.17 ± 0.02 M _J , and a radius of 0.810 ± 0.005 R _J . It is the first warm exo-Saturn with a precisely determined mass and radius. The TESS and ASTEP transits show strong transit timing variations (TTVs), pointing to the existence of a second planet in the system. The joint analysis of the RVs and TTVs provides a unique solution for the nontransiting companion TOI-199 c, which has a period of ${273.69}_{-0.22}^{+0.26}\,{\rm{days}}$ and an estimated mass of ${0.28}_{-0.01}^{+0.02}\,{M}_{{\rm{J}}}$ . This period places it within the conservative habitable zone.

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