| Vergeben? | Thema | Betreuer |
| nein | Cosmological inference (Exposé) | Grandis Sebastian |
| ja | The Crab nebula seen by H.E.S.S. and Fermi-LAT with open-source tools (Exposé) |
Holler Markus and Martí-Devesa Guillem 2) |
| ja | The Pulsar Wind Nebula MSH15-52 as seen with H.E.S.S. and Fermi-LAT |
Holler Markus and Martí-Devesa Guillem |
| nein | Accuracy of telluric corrections in infrared wavelengths, and determination of fractions and time courses in greenhouse trace gas searches (CO2, CH4, …). (Exposé) | Kimeswenger Stefan 1) |
| nein | Modeling the observations of Planetary Nebulae (Exposé) | Kimeswenger Stefan 1) |
| nein | ECHELLE spectra at our observatory: Technique and application to the variability of the red supergiant α Orionis (aka Betelgeuse) since the deep minimum Jan/Feb 2020 to present. (Exposé) | Kimeswenger Stefan 1) |
| ja |
Growth of Instabilities in Shear Flows (Exposé) |
Kissmann Ralf |
| ja | Impact of a Galactic Wind on Cosmic-Ray Transport (Exposé) |
Kissmann Ralf |
| ja | Messungen der Zerfallsbreite des Higgs-Teilchens (Exposé) |
Kneringer Emmerich |
| nein | Globular clusters in ultra diffuse galaxies (Exposé) |
Marleau Francine |
| nein | Nuclear star cluster formation in dwarf galaxies (Exposé) | Marleau Francine |
| ja | Neutrinos from colliding stellar winds (Exposé) |
Martí-Devesa Guillem |
| ja | Anisotropic inverse Compton from Cygnus X-1 (Exposé) |
Martí-Devesa Guillem |
| nein | Argon abundances in hot stars (Exposé) |
Przybilla Norbert |
| nein | Quantitative spectal analysis of the exoplanet host star HIP99770 (Exposé) | Przybilla Norbert |
| nein | Weak gravitational lensing by galaxy clusters (Exposé) | Schrabback Tim and Grandis Sebastian |
| nein | Galaxy distribution in massive clusters (Exposé) |
Schrabback Tim and Grandis Sebastian |
| ja | Galaxy images generated with AI (Exposé) |
Schrabback Tim and Grandis Sebastian |
| ja |
Photometric study of the Orion Nebula Cluster with data from the TESS satellite (Exposé) |
Zwintz Konstanze |
| ja |
Young δ Scuti stars observed with the TESS satellite in long cadence and short cadence (Exposé) |
Zwintz Konstanze |
1) Bemerkung: Nimmt normalerweise maximal EINE Betreuung pro Semester an.
2) New topics could be arranged on demand