Astrobiology16- Page

Representation of metadata factors grouped as environmental factors, operational constraints, experimental design, and assay type for dataset GLDS-37. We exclude the metadata categories that were not populated for this dataset.

Homöller plots of the time- and horizontal-mean vertical profiles of equivalent potential temperature (colors) in each constant-𝛽 simulation. Values from within the model sponge layer are not shown. The black

Simulated stellar wind of TOI-1860, DS Tuc A, and HD 63433 in the x⋆ −y⋆ plane. The rotation axis lies along the positive z⋆. The Alfvén surface is shown as

Weighted mean abundance differences (large–small planet hosts) as a function of the chosen radius cutoff. Colored curves trace the various composite indices, with shaded bands showing uncertainties. The apparent volatile

Retrieved and training disk parameters for Earth-analogues. Left: single-planet per disk; Center: nominal, Right: two-planet systems. Training data is shown if both the planet mass and semi-major axis lies within

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