Confirmation and Characterization of the Eccentric, Warm Jupiter TIC 393818343 b with a Network of Citizen Scientists

NASA’s Transiting Exoplanet Survey Satellite (TESS) has identified over 7000 candidate exoplanets via the transit method, with gas giants among the most readily detected due to their large radii. Even so, long intervals between TESS observations for much of the sky lead to candidates for which only...

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Autors principals:	Lauren A. Sgro, Paul A. Dalba, Thomas M. Esposito, Franck Marchis, Diana Dragomir, Steven Villanueva Jr., Benjamin Fulton, Mario Billiani, Margaret Loose, Nicola Meneghelli, Darren Rivett, Fadi Saibi, Sophie Saibi, Bryan Martin, Georgios Lekkas, Daniel Zaharevitz, Robert T. Zellem, Ivan A. Terentev, Robert Gagliano, Thomas Lee Jacobs, Martti H. Kristiansen, Daryll M. LaCourse, Mark Omohundro, Hans M. Schwengeler
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2024-01-01
Col·lecció:	The Astronomical Journal
Matèries:	Extrasolar gaseous giant planets Transit photometry Exoplanet astronomy Amateur astronomers Amateur astronomy Radial velocity
Accés en línia:	https://doi.org/10.3847/1538-3881/ad5096
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