Astrobiology91- Page

Simulated light curves for triple-lens systems where at least one planet lies in the resonant regime, as defined by the massratio-dependent boundaries (Equations 7) These configurations generally show strong central

Tricorders & Sensors Status Report Rapid Communications In Mass Spectrometry via PubMed December 27, 2025 Computer-aided design (CAD) model cross section of the MIP-MS prototype constructed for this study, including

Planet Venus: Japan’s Venus Climate Orbiter Ultraviolet View December 23, 2016 – JAXA Context: Planets in the HZ can have dense atmospheres affecting their rotations. Over time, the rotation tends

The different views of B3LYP-D3(BJ)/6- 311++G(d,p) level optimized geometric structures for 9- iminofluorene (left) and benzophenone imine (right). The arrow shows C9 position of iminofluorene. — astro-ph.GA Interstellar detections of

TESS target pixel file images of TOI-2094 (LEFT) and TOI-7166 (RIGHT). The red circles are sources identified by Gaia DR3 catalogue (Gaia Collaboration et al. 2016, 2023), labelled with numbers

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