| 19 May 2017 | Advection of potential temperature in the atmosphere of irradiated exoplanets: a robust mechanism to explain radius inflation
| Tremblin, P; Chabrier, G; Mayne, NJ; et al. |
| 15 November 2017 | Cloudless atmospheres for young low-gravity substellar objects
| Tremblin, P; Chabrier, G; Baraffe, I; et al. |
| 16 October 2016 | The effects of consistent chemical kinetics calculations on the pressure-temperature profiles and emission spectra of hot Jupiters
| Drummond, B; Tremblin, P; Baraffe, I; et al. |
| 16 October 2016 | The effects of consistent chemical kinetics calculations on the pressure-temperature profiles and emission spectra of hot Jupiters
| Drummond, B; Tremblin, P; Baraffe, I; et al. |
| 14 March 2019 | Erratum: A library of ATMO forward model transmission spectra for hot Jupiter exoplanets
| Goyal, J; Mayne, N; Sing, D; et al. |
| 12 May 2017 | HAT-P-26b: A Neptune-mass exoplanet with a well-constrained heavy element abundance
| Wakeford, HR; Sing, DK; Kataria, T; et al. |
| 23 November 2017 | A library of ATMO forward model transmission spectra for hot Jupiter exoplanets
| Goyal, JM; Mayne, N; Sing, DK; et al. |
| 3 June 2016 | Near-Infrared Spectroscopy of the Y0 WISEP J173835.52+273258.9 and the Y1 WISE J035000.32-565830.2: the Importance of Non-Equilibrium Chemistry
| Leggett, SK; Tremblin, P; Saumon, D; et al. |
| 4 October 2016 | Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models
| Amundsen, DS; Tremblin, P; Manners, J; et al. |
| 26 August 2016 | The UK Met Office GCM with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b
| Amundsen, DS; Mayne, NJ; Baraffe, I; et al. |
| 26 August 2016 | The UK Met Office GCM with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b
| Amundsen, DS; Mayne, NJ; Baraffe, I; et al. |
| 2 August 2017 | An ultrahot gas-giant exoplanet with a stratosphere
| Evans, T; Sing, D; Kataria, T; et al. |
| 18 December 2014 | Using the UM dynamical cores to reproduce idealised 3-D flows
| Mayne, NJ; Baraffe, I; Acreman, DM; et al. |
