We report on the discovery and validation of TOI 813 b (TIC55525572b), a transiting exoplanet identified by citizen scientists in data from NASA's Transiting Exoplanet Survey Satellite (TESS) and the first planet discovered by the Planet Hunters TESS project. The host star is a bright (V = 10.3 mag) subgiant (R* = 1.94 R☉, M☉ = 1.32 M☉). It was observed almost continuously by TESS during its first year of operations, during which time four individual transit events were detected. The candidate passed all the standard light curve-based vetting checks, and ground-based follow-up spectroscopy and speckle imaging enabled us to place an upper limit of 2 MJup (99 per cent confidence) on the mass of the companion, and to statistically validate its planetary nature. Detailed modelling of the transits yields a period of 83.8911+0.0027-0.0031 d, a planet radius of 6.71 ± 0.38 R⊕ and a semimajor axis of 0.423+0031-0.037 AU. The planet's orbital period combined with the evolved nature of the host star places this object in a relatively underexplored region of parameter space. We estimate that TOI 813 b induces a reflex motion in its host star with a semi-amplitude of ∼6 m s−1, making this a promising system to measure the mass of a relatively long-period transiting planet.

Planet Hunters Tess I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit

Gandolfi D.;Wang J.;Mitchell T.;
2020-01-01

Abstract

We report on the discovery and validation of TOI 813 b (TIC55525572b), a transiting exoplanet identified by citizen scientists in data from NASA's Transiting Exoplanet Survey Satellite (TESS) and the first planet discovered by the Planet Hunters TESS project. The host star is a bright (V = 10.3 mag) subgiant (R* = 1.94 R☉, M☉ = 1.32 M☉). It was observed almost continuously by TESS during its first year of operations, during which time four individual transit events were detected. The candidate passed all the standard light curve-based vetting checks, and ground-based follow-up spectroscopy and speckle imaging enabled us to place an upper limit of 2 MJup (99 per cent confidence) on the mass of the companion, and to statistically validate its planetary nature. Detailed modelling of the transits yields a period of 83.8911+0.0027-0.0031 d, a planet radius of 6.71 ± 0.38 R⊕ and a semimajor axis of 0.423+0031-0.037 AU. The planet's orbital period combined with the evolved nature of the host star places this object in a relatively underexplored region of parameter space. We estimate that TOI 813 b induces a reflex motion in its host star with a semi-amplitude of ∼6 m s−1, making this a promising system to measure the mass of a relatively long-period transiting planet.
2020
494
1
750
763
https://academic.oup.com/mnras/article/494/1/750/5714758
Methods: statistical; Planets and satellites: detection; Stars: fundamental parameters; Stars: individual (TIC-55525572 - TOI 813)
Eisner N.L.; Barragan O.; Aigrain S.; Lintott C.; Miller G.; Zicher N.; Boyajian T.S.; Briceno C.; Bryant E.M.; Christiansen J.L.; Feinstein A.D.; Flor-Torres L.M.; Fridlund M.; Gandolfi D.; Gilbert J.; Guerrero N.; Jenkins J.M.; Jones K.; Kristiansen M.H.; Vanderburg A.; Law N.; Lopez-Sanchez A.R.; Mann A.W.; Safron E.J.; Schwamb M.E.; Stassun K.G.; Osborn H.P.; Wang J.; Zic A.; Ziegler C.; Barnet F.; Bean S.J.; Bundy D.M.; Chetnik Z.; Dawson J.L.; Garstone J.; Stenner A.G.; Huten M.; Larish S.; Melanson L.D.; Mitchell T.; Moore C.; Peltsch K.; Rogers D.J.; Schuster C.; Smith D.S.; Simister D.J.; Tanner C.; Terentev I.; Tsymbal A.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1791031
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