An Informational–Entropic Approach to Exoplanet Characterization
https://www.mdpi.com/1099-4300/27/4/385

Rotating Synthetic Aperture Space Telescope Pointing Control Demonstration and Scalability Analysis
https://arc.aiaa.org/doi/10.2514/1.A36138

Secondary ionisation in hot atmospheres and interactions between planetary and stellar winds
https://www.aanda.org/articles/aa/full_html/2025/04/aa52559-24/aa52559-24.html

Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away
https://iopscience.iop.org/article/10.3847/1538-3881/adbe2f

Photobombing for the Large Interferometer For Exoplanets (LIFE). A New Criterion for Target Confusion and Application to a Mid-infrared Rotating Nulling Interferometer
https://iopscience.iop.org/article/10.3847/1538-3881/adbe6c

The TESS–Keck Survey. XXIV. Outer Giants May Be More Prevalent in the Presence of Inner Small Planets
https://iopscience.iop.org/article/10.3847/1538-3881/adbbed

Eclipse Mapping with MIRI: 2D Map of HD 189733b from 8 μm JWST MIRI LRS Observations
https://iopscience.iop.org/article/10.3847/2041-8213/adc096

HD163296 and its giant planets: Creation of exo-comets, interstellar objects and transport of volatile material
https://www.researchgate.net/publication/390462606_HD163296_and_its_giant_planets_Creation_of_exo-comets_interstellar_objects_and_transport_of_volatile_material

Planet Earth in reflected and polarized light I. 3D radiative transfer simulations of realistic surface-atmosphere systems
https://arxiv.org/abs/2504.02048

An MHD Simulation of the Possible Modulations of Stellar CMEs Radio Observations by an Exoplanetary Magnetosphere
https://arxiv.org/abs/2504.02469

Helium escape signatures are generally strongest during younger ages but this age dependence is lost in the diversity of observed exoplanets
https://arxiv.org/abs/2504.02578

Cosmic ray ionisation of a post-impact early Earth atmosphere: Solar cosmic ray ionisation must be considered in origin-of-life scenarios
https://arxiv.org/abs/2504.02596

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