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)
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.