Planet Hunters TESS I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit
| dc.contributor.author | Eisner, N L | |
| dc.contributor.author | Barragan, O | |
| dc.contributor.author | Aigrain, Suzanne | |
| dc.contributor.author | Lintott, Chris J. | |
| dc.contributor.author | Miller, G | |
| dc.contributor.author | Zicher, N | |
| dc.contributor.author | Boyajian, Tabetha | |
| dc.contributor.author | Briceno, C | |
| dc.contributor.author | Bryant, E M | |
| dc.contributor.author | Christiansen, Jessie L. | |
| dc.contributor.author | Gilbert, James | |
| dc.date.accessioned | 2023-03-22T00:59:51Z | |
| dc.date.available | 2023-03-22T00:59:51Z | |
| dc.date.issued | 2020 | |
| dc.date.updated | 2022-01-16T07:18:30Z | |
| dc.description.abstract | We report on the discovery and validation of TOI 813 b (TIC 55525572 b), 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+0.031 −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 ∼6ms−1, making this a promising system to measure the mass of a relatively long-period transiting planet | en_AU |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 0035-8711 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/287269 | |
| dc.language.iso | en_AU | en_AU |
| dc.provenance | https://v2.sherpa.ac.uk/id/publication/24618..."The Published Version can be archived in an Institutional Repository" from SHERPA/RoMEO site (as at 22/03/2023). This article has been accepted for publication in [Monthly Notices of the Royal Astronomical Society] ©: 2020 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | en_AU |
| dc.publisher | Oxford University Press | en_AU |
| dc.rights | © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society | en_AU |
| dc.source | Monthly Notices of the Royal Astronomical Society | en_AU |
| dc.subject | methods: statistical | en_AU |
| dc.subject | planets and satellites: detection | en_AU |
| dc.subject | stars: fundamental parameters | en_AU |
| dc.subject | stars: individual (TIC-55525572 – TOI 813) | en_AU |
| dc.title | Planet Hunters TESS I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit | en_AU |
| dc.type | Journal article | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.issue | 1 | en_AU |
| local.bibliographicCitation.lastpage | 763 | en_AU |
| local.bibliographicCitation.startpage | 750 | en_AU |
| local.contributor.affiliation | Eisner, N L, University of Oxford | en_AU |
| local.contributor.affiliation | Barragan, O, University of Oxford | en_AU |
| local.contributor.affiliation | Aigrain, Suzanne, University of Oxford | en_AU |
| local.contributor.affiliation | Lintott, Chris J., University of Oxford | en_AU |
| local.contributor.affiliation | Miller, G, University of Oxford | en_AU |
| local.contributor.affiliation | Zicher, N, University of Oxford | en_AU |
| local.contributor.affiliation | Boyajian, Tabetha, Louisiana State University | en_AU |
| local.contributor.affiliation | Briceno, C, Cerro Tololo Inter-American Observatory | en_AU |
| local.contributor.affiliation | Bryant, E M, University of Warwick | en_AU |
| local.contributor.affiliation | Christiansen, Jessie L., Caltech/IPAC-NASA Exoplanet Science Institute | en_AU |
| local.contributor.affiliation | Gilbert, James, College of Science, ANU | en_AU |
| local.contributor.authoruid | Gilbert, James, u1022755 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.identifier.absfor | 510109 - Stellar astronomy and planetary systems | en_AU |
| local.identifier.absfor | 510107 - Planetary science (excl. solar system and planetary geology) | en_AU |
| local.identifier.absseo | 280120 - Expanding knowledge in the physical sciences | en_AU |
| local.identifier.ariespublication | a383154xPUB13641 | en_AU |
| local.identifier.citationvolume | 494 | en_AU |
| local.identifier.doi | 10.1093/mnras/staa138 | en_AU |
| local.publisher.url | https://academic.oup.com/mnras | en_AU |
| local.type.status | Published Version | en_AU |
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