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 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.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).