Modelling Terrestrial and Potential Extraterrestrial Photopigments via Density Functional Theory
https://repository.fit.edu/etd/1425/
Activity of the Star TOI-784 and Loss of Atmospheric Mass by Its Planet
https://link.springer.com/article/10.1007/s10511-024-09815-4
Mass Loss from the Atmosphere of the Planet TOI-1442 c
https://link.springer.com/article/10.1007/s10511-024-09816-3
Feature extraction for exoplanet detection
https://link.springer.com/article/10.1007/s41060-024-00552-7
Signature of the atmospheric asymmetries of hot and ultra-hot Jupiters in light curves
https://www.aanda.org/articles/aa/full_html/2024/05/aa48880-23/aa48880-23.html
Star-spot activity, orbital obliquity, transmission spectrum, physical properties, and transit time variations of the HATS-2 planetary system
https://www.aanda.org/articles/aa/full_html/2024/05/aa47872-23/aa47872-23.html
The Mantis Network – IV. A titanium cold trap on the ultra-hot Jupiter WASP-121 b
https://www.aanda.org/articles/aa/full_html/2024/05/aa44968-22/aa44968-22.html
Planets similar in size are often dissimilar in interior
https://www.aanda.org/articles/aa/full_html/2024/05/aa47049-23/aa47049-23.html
Secular evolution of resonant planets in the coplanar case – Application to the systems HD 73526 and HD 31527
https://www.aanda.org/articles/aa/full_html/2024/05/aa48378-23/aa48378-23.html
Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Subprime Field Planets
https://iopscience.iop.org/article/10.3847/1538-3881/ad3ba3
The Impact-driven Atmospheric Loss of Super-Earths around Different Spectral Types of Host Stars
https://iopscience.iop.org/article/10.3847/1538-4357/ad3af9
Dark Matter Halo Parameters from Overheated Exoplanets via Bayesian Hierarchical Inference
https://arxiv.org/abs/2405.09578
Dynamical coupling of Keplerian orbits in a hierarchical four-body system: from the Galactic Centre to compact planetary systems
https://arxiv.org/abs/2405.09630
The metallicity and carbon-to-oxygen ratio of the ultra-hot Jupiter WASP-76b from Gemini-S/IGRINS
https://arxiv.org/abs/2405.09769
How planets form by pebble accretion V. Silicate rainout delays contraction of sub-Neptunes
https://arxiv.org/abs/2405.09900