(Top) A simulated transit depth spectrum showing SF6 and NF3 in the atmosphere of terrestrial exoplanets of different atmospheric compositions orbiting an M Dwarf star. The concentrations of SF6 and

This system integrates Akatsuki observation data and AFES-Venus numerical simulation forecast data using the LETKF data assimilation method. The release of ALERA-V, objective analysis data that spatiotemporally reconstructs a more

Phase folded best-fit transit models of TOI-4311b( purple) and TOI-4311c (green) with the underlying TESS (left) and CHEOPS (right) data in black in the top panel. The residuals are shown

The Mars rover with its innovative wheels, which can ‘swim’ through sand, modelled on a desert lizard. (Image: Marco Schmidt / Universität Würzburg) Some animals can move efficiently beneath granular

Declination of the 50 targets presenting the largest RSM′ values as a function of their respective score. The ten most favourable targets are annotated with their names. The areas of