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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06182naa a2200997 4500 | |
| 001 | oai:research.chalmers.se:700c5b9d-e769-4312-86e6-bb1b0c933971 | |
| 003 | SwePub | |
| 008 | 200602s2020 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://doi.org/10.1093/mnras/staa1382 DOI |
| 024 | 7 | a https://research.chalmers.se/publication/5172872 URI |
| 040 | a (SwePub)cth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a for2 swepub-publicationtype |
| 072 | 7 | a ref2 swepub-contenttype |
| 100 | 1 | a Eisner, N. L.u University Of Oxford4 aut |
| 245 | 1 0 | a Planet Hunters Tess I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit |
| 264 | c 2020-01-23 | |
| 264 | 1 | b Oxford University Press (OUP),c 2020 |
| 338 | a electronic2 rdacarrier | |
| 520 | a 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. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 650 | 7 | a NATURVETENSKAPx Geovetenskap och miljövetenskapx Geofysik0 (SwePub)105052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Geophysics0 (SwePub)105052 hsv//eng |
| 653 | a Stars: fundamental parameters | |
| 653 | a Stars: individual (TIC-55525572 - TOI 813) | |
| 653 | a Methods: statistical | |
| 653 | a Planets and satellites: detection | |
| 700 | 1 | a Barragán, O.u University Of Oxford4 aut |
| 700 | 1 | a Aigrain, S.u University Of Oxford4 aut |
| 700 | 1 | a Lintott, C.u University Of Oxford4 aut |
| 700 | 1 | a Miller, G.u University Of Oxford4 aut |
| 700 | 1 | a Zicher, N.u University Of Oxford4 aut |
| 700 | 1 | a Boyajian, T. S.u Louisiana State University4 aut |
| 700 | 1 | a Briceño, C.4 aut |
| 700 | 1 | a Bryant, E.u The University of Warwick4 aut |
| 700 | 1 | a Christiansen, J. L.u NASA Ames Research Center4 aut |
| 700 | 1 | a Feinstein, A. D.u University of Chicago4 aut |
| 700 | 1 | a Flor-Torres, L. M.u Universidad de Guanajuato4 aut |
| 700 | 1 | a Fridlund, Malcolm,d 1952u Chalmers tekniska högskola,Chalmers University of Technology,Universiteit Leiden (UL),Leiden University (UL)4 aut0 (Swepub:cth)malfri |
| 700 | 1 | a Gandolfi, D.u Universita degli Studi di Torino,University of Turin4 aut |
| 700 | 1 | a Gilbert, J.u Australian National University4 aut |
| 700 | 1 | a Guerrero, N.u Massachusetts Institute of Technology (MIT)4 aut |
| 700 | 1 | a Jenkins, Jon M.u NASA Ames Research Center4 aut |
| 700 | 1 | a Jones, K.u University Of Oxford4 aut |
| 700 | 1 | a Kristiansen, M. H.u Danmarks Tekniske Universitet,Technical University of Denmark4 aut |
| 700 | 1 | a Vanderburg, A.u The University of Texas at Austin, USA4 aut |
| 700 | 1 | a Law, N.u The University of North Carolina System4 aut |
| 700 | 1 | a López-Sánchez, A. R.u Macquarie University4 aut |
| 700 | 1 | a Mann, A.u The University of North Carolina System4 aut |
| 700 | 1 | a Safron, E. J.u Louisiana State University4 aut |
| 700 | 1 | a Schwamb, M. E.u Queen's University Belfast,Gemini Observatory North4 aut |
| 700 | 1 | a Stassun, Keivan G.u Vanderbilt University,Fisk University4 aut |
| 700 | 1 | a Osborn, H. P.u Laboratoire d'Astrophysique de Marseille4 aut |
| 700 | 1 | a Wang, J.u Yale University4 aut |
| 700 | 1 | a Zic, A.u Commonwealth Scientific and Industrial Research Organisation (CSIRO),The University of Sydney4 aut |
| 700 | 1 | a Ziegler, C.u University of Toronto4 aut |
| 700 | 1 | a Barnet, F.4 aut |
| 700 | 1 | a Bean, S. J.4 aut |
| 700 | 1 | a Bundy, D. M.4 aut |
| 700 | 1 | a Chetnik, Z.4 aut |
| 700 | 1 | a Dawson, J. L.4 aut |
| 700 | 1 | a Garstone, J.4 aut |
| 700 | 1 | a Stenner, A. G.4 aut |
| 700 | 1 | a Huten, M.4 aut |
| 700 | 1 | a Larish, S.4 aut |
| 700 | 1 | a Melanson, L. D.4 aut |
| 700 | 1 | a Mitchell, T.4 aut |
| 700 | 1 | a Moore, C.4 aut |
| 700 | 1 | a Peltsch, K.4 aut |
| 700 | 1 | a Rogers, D. J.4 aut |
| 700 | 1 | a Schuster, C.4 aut |
| 700 | 1 | a Smith, D. S.4 aut |
| 700 | 1 | a Simister, D. J.4 aut |
| 700 | 1 | a Tanner, C.4 aut |
| 700 | 1 | a Terentev, I.4 aut |
| 700 | 1 | a Tsymbal, A.4 aut |
| 710 | 2 | a University Of Oxfordb Louisiana State University4 org |
| 773 | 0 | t Monthly Notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 494:1, s. 750-763q 494:1<750-763x 0035-8711x 1365-2966 |
| 856 | 4 | u https://research.chalmers.se/publication/517287/file/517287_Fulltext.pdfx primaryx freey FULLTEXT |
| 856 | 4 | u https://digitalcommons.lsu.edu/cgi/viewcontent.cgi?article=1465&context=physics_astronomy_pubs |
| 856 | 4 8 | u https://doi.org/10.1093/mnras/staa138 |
| 856 | 4 8 | u https://research.chalmers.se/publication/517287 |
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