Structures and relative energy levels of cis-HNSO (left, as the ground state), trans-HNSO (right, at 3.7 kcal/mol), and the transition state (middle, at 14.5 kcal/mol); energy values were derived by

Plot of the Habitable Zone (HZ) completeness as a function of host star luminosity (in units of Solar luminosity) and distance (in parsecs). Here the AYO results are on the

Artistic representation of the collision of two planetesimals in the circumstellar disc of the star Fomalhaut. Credit Thomas Müller (MPIA) Young star systems are a place of violent collisions. Rocks,

Comparison result between the DBSCAN algorithm and the KNN algorithm for residual RFI mitigation. Data points marked in red represent signals identified and removed as residual RFI, while those in

The transmission spectrum of TOI-732 c in the NIR. We show the spectrum and retrieved model fits for the one-offset retrieval, as discussed in Section 3.3. This model includes the

Schematic loosely sketching the parameter space accessible using the astrometric technique as compared to the transit methods of exomoon detection in the context of the moon survival rate as a