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arXiv 2005.01684astro-ph.EPphysics.ed-ph
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Original Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets

Billy Edwards, Quentin Changeat, Kai Hou Yip, Angelos Tsiaras, Jake Taylor, Bilal Akhtar, Josef AlDaghir, Pranup Bhattarai, Tushar Bhudia, Aashish Chapagai, Mic… 展开作者

Billy Edwards, Quentin Changeat, Kai Hou Yip, Angelos Tsiaras, Jake Taylor, Bilal Akhtar, Josef AlDaghir, Pranup Bhattarai, Tushar Bhudia, Aashish Chapagai, Michael Huang, Danyaal Kabir, Vieran Khag, Summyyah Khaliq, Kush Khatri, Jaidev Kneth, Manisha Kothari, Ibrahim Najmudin, Lobanaa Panchalingam, Manthan Patel, Luxshan Premachandran, Adam Qayyum, Prasen Rana, Zain Shaikh, Sheryar Syed, Harnam Theti, Mahmoud Zaidani, Manasvee Saraf, Damien de Mijolla, Hamish Caines, Anatasia Kokori, Marco Rocchetto, Matthias Mallonn, Matthieu Bachschmidt, Josep M. Bosch, Marc Bretton, Philippe Chatelain, Marc Deldem, Romina Di Sisto, Phil Evans, Eduardo Fernandez-Lajus, Pere Guerra, Ferran Grau Horta, Wonseok Kang, Taewoo Kim, Arnaud Leroy, Frantivsek Lomoz, Juan Lozano de Haro, Veli-Pekka Hentunen, Yves Jongen, David Molina, Romain Montaigut, Ramon Naves, Manfred Raetz, Thomas Sauer, Americo Watkins, Anael Wunsche, Martin Zibar, William Dunn, Marcell Tessenyi, Giorgio Savini, Giovanna Tinetti, Jonathan Tennyson

英文摘要:

We report follow-up observations of transiting exoplanets that have either large uncertainties (>10 minutes) in their transit times or have not been observed for over three years. A fully robotic ground-based telescope network, observations from citizen astronomers and data from TESS have been used to study eight planets, refining their ephemeris and orbital data. Such follow-up observations are key for ensuring accurate transit times for upcoming ground and space-based telescopes which may seek to characterise the atmospheres of these planets. We find deviations from the expected transit time for all planets, with transits occurring outside the 1 sigma uncertainties for seven planets. Using the newly acquired observations, we subsequently refine their periods and reduce the current predicted ephemeris uncertainties to 0.28 - 4.01 minutes. A significant portion of this work has been completed by students at two high schools in London as part of the Original Research By Young Twinkle Students (ORBYTS) programme.

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