HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS

@article{Wang2019HD2B,
  title={HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS},
  author={S. Wang and M. Jones and A. Shporer and B. Fulton and L. Paredes and T. Trifonov and D. Kossakowski and J. Eastman and M. Gunther and C. Huang and S. Millholland and Darryl Seligman and D. Fischer and R. Brahm and Xian-yu Wang and B. Cruz and H. James and B. Addison and T. Henry and E. Liang and A. B. Davis and R. Tronsgaard and Keduse Worku and J. Brewer and M. Kurster and C. Beichman and A. Bieryla and T. Brown and J. Christiansen and D. Ciardi and K. Collins and G. Esquerdo and A. Howard and H. Isaacson and D. Latham and T. Mazeh and E. Petigura and S. Quinn and S. Shahaf and R. Siverd and G. Ricker and R. Vanderspek and S. Seager and J. Winn and J. Jenkins and P. Boyd and G. Fur'esz and C. Henze and A. M. Levine and J. Morris and M. Paegert and K. Stassun and E. Ting and Michael L. Vezie and G. Laughlin},
  journal={The Astronomical Journal},
  year={2019},
  volume={157},
  pages={51-51}
}
  • S. Wang, M. Jones, +52 authors G. Laughlin
  • Published 2019
  • Physics
  • The Astronomical Journal
  • We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days… CONTINUE READING
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