Nathan J. Mayne

TL;DR: In this article, the authors used the Xgrid facilities at the University of Exeter to reduce the photometric data presented in this study, which were used to improve the results and conclusions of the paper.

TL;DR: In this paper, the authors collected and summarized the magnetic field topology information obtained to date and presented Hertzsprung-Russell (H-R) diagrams for the stars in the sample.

TL;DR: In this paper, the authors demonstrate the successful adaptation of the most sophisticated dynamical core, the component of the GCM which solves the equations of motion for the atmosphere, available within the EndGame (Even Newer Dynamics for General atmospheric modelling of the environment).

TL;DR: In this article, the authors adapted the UK Met Office GCM, the Unified Model (UM), for the study of hot Jupiters, and presented the adaptation of the Edwards-Slingo radiation scheme based on the two-stream approximation and the correlated-k method.

TL;DR: In this article, the authors used several main-sequence models to derive distances and extinctions, with statistically meaningful uncertainties for 11 star-forming regions and young clusters, and they used a feature called radiative-convective gap overlap to provide a diagnostic of isochronal age spreads or varying accretion histories within a given star formation region.