Alshehhi, R.; Rodenbeck, K.; Gizon, L.; Sreenivasan, K. R.: Detection of exomoons in simulated light curves with a regularized convolutional neural network. Astronomy and Astrophysics 640, A41 (2020)
Heller, R.; Hippke, M.; Rodenbeck, K.: Transit least-squares survey: II. Discovery and validation of 17 new sub- to super-Earth-sized planets in multi-planet systems from K2. Astronomy and Astrophysics 627, A66 (2019)
Heller, R.; Rodenbeck, K.; Bruno, G.: An alternative interpretation of the exomoon candidate signal in the combined Kepler and Hubble data of Kepler-1625. Astronomy and Astrophysics 624, A95 (2019)
Heller, R.; Rodenbeck, K.; Hippke, M.: Transit least-squares survey: I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance. Astronomy and Astrophysics 625, A31 (2019)
Lanza, A. F.; Gizon, L.; Zaqarashvili, T. V.; Liang, Z.-C.; Rodenbeck, K.: Sectoral r modes and periodic radial velocity variations of Sun-like stars. Astronomy and Astrophysics 623, A50 (2019)
Rodenbeck, K.; Heller, R.; Hippke, M.; Gizon, L.: Revisiting the exomoon candidate signal around Kepler 1625 b. Astronomy and Astrophysics 617, A49 (2018)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...