Müller, B.; Hohage, T.; Fournier, D.; Gizon, L.: Quantitative passive imaging by iterative holography: the example of helioseismic holography. Inverse Problems 40, p. 045016 (2024)
Müller, B.; Hohage, T.; Fournier, D.; Gizon, L.: Quantitative passive imaging by iterative holography: the example of helioseismic holography. Inverse Problems 40, p. 045016 (2024)
Kollatschny, W.; Ochmann, M. W.; Kaspi, S.; Schumacher, C.; Behar, E.; Chelouche, D.; Horne, K.; Müller, B.; Rafter, S. E.; Chini, R.et al.; Haas, M.; Probst, M. A.: The Great Slump: Mrk 926 reveals discrete and varying Balmer line satellite components during a drastic phase of decline. Astronomy and Astrophysics 657, p. A122 (2022)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.