Beyond Homochirality: Computer Modeling Hints of Heterochiral Proteins in Early and Extraterrestrial Life
https://liebertpub.com/doi/10.1089/ast.2024.0072

The Role of Atmospheric Composition in Defining the Habitable Zone Limits and Supporting E. coli Growth
https://www.mdpi.com/2075-1729/15/1/79

A new pathway to SO2 – Revealing the NUV driven sulfur chemistry in hot gas giants
https://www.aanda.org/articles/aa/full_html/2025/01/aa50598-24/aa50598-24.html

Most High-density Exoplanets Are Unlikely to Be Remnant Giant Planet’s Cores
https://iopscience.iop.org/article/10.3847/2041-8213/ad86c3

Semiclassical Estimates of Pressure-induced Line Widths for Infrared Absorption in Hot (Exo)planetary Atmospheres
https://iopscience.iop.org/article/10.3847/1538-4365/ad9b19

Oxidizing ExoCAM: Introducing the Radiative Effects of Oxygen and Ozone into the ExoCAM General Circulation Model
https://iopscience.iop.org/article/10.3847/PSJ/ad9900

Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-Hydrodynamic Code
https://arxiv.org/abs/2501.04834

The CO-Fuelled Time Machine: Tracing Birth Conditions and Terrestrial Planet Formation Outcomes in HD 163296 through Pebble Drift-induced CO Enhancements
https://arxiv.org/abs/2501.05316

A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star
https://arxiv.org/abs/2501.05431

Network and Kinetics-based Biosignatures: Implications for the Putative Habitable World Observatory Design
https://arxiv.org/abs/2501.04737

Identifying Flare Locations Through Exoplanet Transit Occultations
https://arxiv.org/abs/2501.04866

High-resolution imaging of the radio source associated with Project Hephaistos Dyson Sphere Candidate G
https://arxiv.org/abs/2501.05152

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