年轻的Twinkle学生（ORBYTS）的原始研究：迁移系外行星II

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年轻的Twinkle学生（ORBYTS）的原始研究：迁移系外行星II

Original Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets II

论文作者

Edwards, Billy, Anisman, Lara, Changeat, Quentin, Morvan, Mario, Wright, Sam, Yip, Kai Hou, Abdullahi, Amiira, Ali, Jesmin, Amofa, Clarry, Antoniou, Antony, Arzouni, Shahad, Bradley, Noeka, Campana, Dayanara, Chavda, Nandini, Creswell, Jessy, Gazieva, Neliman, Gudgeon-Sidelnikova, Emily, Guha, Pratap, Hayden, Ella, Huda, Mohammed, Hussein, Hana, Ibrahim, Ayub, Ike, Chika, Jama, Salma, Joshi, Bhavya, Kc, Schet, Keenan, Paris, Kelly-Smith, Charlie, Khan, Aziza, Korodimos, George, Liang, Jiale, Nogueira, Guilherme Luis, Martey-Botchway, Neil, Masruri, Asan, Miyamaru, Osuke, Moalin, Ismail, Monteiro, Fabiana, Nawrocka, Adrianna, Musa, Sebri, Nelson, Lilith, Ogunjuyigbe, Isabel, Patel, Jaymit, Pereira, Joesph, Ramsey, James, Rasoul, Billnd, Reetsong, Tumo, Saeed, Haad, Sander, Cameron, Sanetra, Matthew, Tarabe, Zainab, Tareke, Milcah, Tasneem, Nazifa, Teo, Meigan, Uddin, Asiyah, Upadhyay, Kanvi, Yanakiev, Kaloyan, Yatingiri, Deepakgiri, Dunn, William, Kokori, Anatasia, Tsiaras, Angelos, Gomez, Edward, Tinetti, Giovanna, Tennyson, Jonathan

论文摘要

我们报告了四个过渡系外行星，TRE-2B，HAT-P-22B，HAT-P-36B和XO-2B的后续观察，这是年轻Twinkle学生（Orbyts）计划的原始研究的一部分。使用Las Cumbres天文台全球望远镜网络（LCOGT）机器人0.4 M望远镜进行这些观察结果，并使用Holomon光度计软件（HOPS）分析。此类观察是确保即将到来的望远镜的准确运输时间的关键，例如James Webb太空望远镜（JWST），Twinkle和Ariel，它们可能试图表征这些星球的气氛。数据已上传到exoclock，这项工作的很大一部分已由伦敦的中学生完成。

We report follow-up observations of four transiting exoplanets, TRES-2b, HAT-P-22b, HAT-P-36b and XO-2b, as part of the Original Research By Young Twinkle Students (ORBYTS) programme. These observations were taken using the Las Cumbres Observatory Global Telescope Network's (LCOGT) robotic 0.4 m telescopes and were analysed using the HOlomon Photometric Software (HOPS). Such observations are key for ensuring accurate transit times for upcoming telescopes, such as the James Webb Space Telescope (JWST), Twinkle and Ariel, which may seek to characterise the atmospheres of these planets. The data have been uploaded to ExoClock and a significant portion of this work has been completed by secondary school students in London.

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