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Norton, Andrew; Dickinson, Hugh; McMaster, Adam; Middleton, Matthew and West, Richard
(2022).
DOI: https://doi.org/10.3847/2515-5172/ac6811
Abstract
We present the SuperWASP light curve of a 10th magnitude A7V star containing a single, well-defined U-shaped transit-like event lasting around 11 days with a depth of 1.1%. The star is otherwise non-variable throughout the 8 yr duration of the observations. If the event is modeled as an exoplanet transit, it is compatible with a 1.8 RJ exoplanet in a ∼205 au orbit with a period of ∼2200 yr.
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About
- Item ORO ID
- 82869
- Item Type
- Journal Item
- Project Funding Details
-
Funded Project Name Project ID Funding Body STFC 2020 DTG S5450 STFC - Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- Astronomy
- Copyright Holders
- © 2022 The Authors
- Depositing User
- Andrew Norton