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| Funder | Science and Technology Facilities Council |
|---|---|
| Recipient Organization | University of Warwick |
| Country | United Kingdom |
| Start Date | Sep 30, 2024 |
| End Date | Mar 30, 2028 |
| Duration | 1,277 days |
| Number of Grantees | 2 |
| Roles | Student; Supervisor |
| Data Source | UKRI Gateway to Research |
| Grant ID | 2926052 |
The project combines transmission spectroscopy observations of transiting exoplanets from ground-based and space-based telescopes to measure the composition of giant planet atmospheres.
In particular, the aim is to detect and exploit spatial inhomogeneities in the planetary atmosphere in order to study global circulation and cloud formation in 2D and maybe 3D.
Observational data will be both high and low spectral resolution, and ground-based data will come primarily from ESO telescopes. We are likely also to include data from JWST and maybe HST.
We will aim to exploit a code called TERMINATOR developed by a fellow at Warwick, as well as other data reduction and modelling codes.
University of Warwick
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