Radial variations in nitrogen, carbon, and hydrogen fractionation in the PDS 70 planet-hosting disk
https://arxiv.org/abs/2504.03833
Formation of Giant Planets
https://arxiv.org/abs/2504.04090
Has DESI detected exponential quintessence?
https://arxiv.org/abs/2504.04226
Bioverse: Potentially Observable Exoplanet Biosignature Patterns Under the UV Threshold Hypothesis for the Origin of Life
https://arxiv.org/abs/2504.04261
How much has DESI dark energy evolved since DR1?
https://arxiv.org/abs/2504.04417
The enigmatic magnetic field of the planet hosting Herbig Ae/Be star HD169142
https://arxiv.org/abs/2504.04439
A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
https://arxiv.org/abs/2504.04646
Formation of Near-surface Atmospheric Inversion and Surface Inversion in Hothouse Climates
https://arxiv.org/abs/2504.05233
What if we Find Nothing? Bayesian Analysis of the Statistical Information of Null Results in Future Exoplanet Habitability and Biosignature Surveys
https://iopscience.iop.org/article/10.3847/1538-3881/adb96d
Helium escape signatures are generally strongest during younger ages but this age dependence is lost in the diversity of observed exoplanets
https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staf566/8107903