The Astrophysical Journal Supplement Series (Jan 2023)

The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets

  • Samuel W. Yee,
  • Joshua N. Winn,
  • Joel D. Hartman,
  • Luke G. Bouma,
  • George Zhou,
  • Samuel N. Quinn,
  • David W. Latham,
  • Allyson Bieryla,
  • Joseph E. Rodriguez,
  • Karen A. Collins,
  • Owen Alfaro,
  • Khalid Barkaoui,
  • Corey Beard,
  • Alexander A. Belinski,
  • Zouhair Benkhaldoun,
  • Paul Benni,
  • Krzysztof Bernacki,
  • Andrew W. Boyle,
  • R. Paul Butler,
  • Douglas A. Caldwell,
  • Ashley Chontos,
  • Jessie L. Christiansen,
  • David R. Ciardi,
  • Kevin I. Collins,
  • Dennis M. Conti,
  • Jeffrey D. Crane,
  • Tansu Daylan,
  • Courtney D. Dressing,
  • Jason D. Eastman,
  • Zahra Essack,
  • Phil Evans,
  • Mark E. Everett,
  • Sergio Fajardo-Acosta,
  • Raquel Forés-Toribio,
  • Elise Furlan,
  • Mourad Ghachoui,
  • Michaël Gillon,
  • Coel Hellier,
  • Ian Helm,
  • Andrew W. Howard,
  • Steve B. Howell,
  • Howard Isaacson,
  • Emmanuel Jehin,
  • Jon M. Jenkins,
  • Eric L. N. Jensen,
  • John F. Kielkopf,
  • Didier Laloum,
  • Naunet Leonhardes-Barboza,
  • Pablo Lewin,
  • Sarah E. Logsdon,
  • Jack Lubin,
  • Michael B. Lund,
  • Mason G. MacDougall,
  • Andrew W. Mann,
  • Natalia A. Maslennikova,
  • Bob Massey,
  • Kim K. McLeod,
  • Jose A. Muñoz,
  • Patrick Newman,
  • Valeri Orlov,
  • Peter Plavchan,
  • Adam Popowicz,
  • Francisco J. Pozuelos,
  • Tyler A. Pritchard,
  • Don J. Radford,
  • Michael Reefe,
  • George R. Ricker,
  • Alexander Rudat,
  • Boris S. Safonov,
  • Richard P. Schwarz,
  • Heidi Schweiker,
  • Nicholas J. Scott,
  • S. Seager,
  • Stephen A. Shectman,
  • Chris Stockdale,
  • Thiam-Guan Tan,
  • Johanna K. Teske,
  • Neil B. Thomas,
  • Mathilde Timmermans,
  • Roland Vanderspek,
  • David Vermilion,
  • David Watanabe,
  • Lauren M. Weiss,
  • Richard G. West,
  • Judah Van Zandt,
  • Michal Zejmo,
  • Carl Ziegler

DOI
https://doi.org/10.3847/1538-4365/aca286
Journal volume & issue
Vol. 265, no. 1
p. 1

Abstract

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NASA’s Transiting Exoplanet Survey Satellite (TESS) mission promises to improve our understanding of hot Jupiters by providing an all-sky, magnitude-limited sample of transiting hot Jupiters suitable for population studies. Assembling such a sample requires confirming hundreds of planet candidates with additional follow-up observations. Here we present 20 hot Jupiters that were detected using TESS data and confirmed to be planets through photometric, spectroscopic, and imaging observations coordinated by the TESS Follow-up Observing Program. These 20 planets have orbital periods shorter than 7 days and orbit relatively bright FGK stars (10.9 < G < 13.0). Most of the planets are comparable in mass to Jupiter, although there are four planets with masses less than that of Saturn. TOI-3976b, the longest-period planet in our sample ( P = 6.6 days), may be on a moderately eccentric orbit ( e = 0.18 ± 0.06), while observations of the other targets are consistent with them being on circular orbits. We measured the projected stellar obliquity of TOI-1937A b, a hot Jupiter on a 22.4 hr orbit with the Rossiter–McLaughlin effect, finding the planet’s orbit to be well aligned with the stellar spin axis (∣ λ ∣ = 4.°0 ± 3.°5). We also investigated the possibility that TOI-1937 is a member of the NGC 2516 open cluster but ultimately found the evidence for cluster membership to be ambiguous. These objects are part of a larger effort to build a complete sample of hot Jupiters to be used for future demographic and detailed characterization work.

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