Original Research By Young Twinkle Students (ORBYTS): Ephemeris Refinement of Transiting Exoplanets III
DOI:
https://doi.org/10.32374/atom.2020.2.4Keywords:
exoplanets, transit photometry, ground telescopes, HATS-1b, HATS-2b, HATS-3b, HAT-P-18b, HAT-P-27b, HAT-P-30b, HAT-P-55b, KELT-4Ab, WASP-25b, WASP-42b, WASP-57b, WASP-61b, WASP-123bAbstract
We report photometric follow-up observations of thirteen exoplanets (HATS-1 b, HATS-2 b, HATS-3 b, HAT-P-18 b, HAT-P-27 b, HAT-P-30 b, HAT-P-55 b, KELT-4A b, WASP-25 b, WASP-42 b, WASP-57 b, WASP-61 b and WASP-123 b), as part of the Original Research By Young Twinkle Students (ORBYTS) programme. All these planets are potentially viable targets for atmospheric characterisation and our data, which were taken using the LCOGT network of ground-based telescopes, will be combined with observations from other users of ExoClock to ensure that the transit times of these planets continue to be well-known, far into the future.
Downloads
Published
Issue
Section
License
Copyright (c) 2021 Billy Edwards, Cynthia Ho, Hannah Osborne, Nabeeha Deen, Ellie Hathorn, Solomon Johnson, Jiya Patel, Varun Vogireddy, Ansh Waddon, Ayuub Ahmed, Muhammad Bham, Nathan Campbell, Zahra Chummun, Nicholas Crossley, Reggie Dunsdon, Robert Hayes, Haroon Malik, Frank Marsden, Lois Mayfield, Liston Mitchell, Agnes Prosser, Valentina Rabrenovic, Emma Smith, Rico Thomas, Anastasia Kokori, Angelos Tsiaras, Marcell Tessenyi, Giovanni Tinetti, Jonathan Tennyson
This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.