Heller, R.; Hippke, M.; Placek, B.; Angerhausen, D.; Agol, E.: Predictable patterns in planetary transit timing variations and transit duration variations due to exomoons. Astronomy and Astrophysics 591, A67 (2016)
Oshagh, M.; Heller, R.; Dreizler, S.: How eclipse time variations, eclipse duration variations and radial velocities can reveal S-type planets in close eclipsing binaries. Mon. Not. Roy. Astron. Soc. 466, pp. 4683 - 4691 (2016)
Heller, R.: Detecting and Characterizing Exomoons and Exorings. In: Handbook of Exoplanets, pp. 835 - 851 (Eds. Deeg, H. J.; Belmonte, J. A.). Springer, Cham (2018)
Heller, R.: New Predictions of PLATO's Yield of Earth-sized Transiting Planets in the Habitable Zone of Sun-like Stars. SPP1992 all-hands-on-deck meeting, Online (2021)
Heller, R.: Analytic Solutions to Exoplanet Transit Depth for Ad Hoc Limb Darkening Laws. Getting Ultra-Precise Planetary Radii with PLATO: The Impact of Limb Darkening and Stellar Activity on Transit Light Curves, Online (2021)
Heller, R.: Habitability of early Earth:Liquid water under a faint young Sunand tidal heating due to a closer Moon. GeoKarlsruhe 2021: Sustainable Earth - from processes to resources, Online (2021)
Heller, R.: Earth-sized Transiting Planets in the Stellar Habitable ZonesFrom Kepler to PLATO. Virtual Annual meeting of the German Astronomical Society, Online (2021)
Heller, R.: Habitability of early Earth: Liquid water under a faint young Sun and tidal heating due to a closer Moon. General Meeting of the SPP 1833 "Building a Habitable Earth", online (2021)
Heller, R.: Challenges of Validating Earth-like Transiting Planets Around Sun-like Stars. Splinter session "Exploring the diversity of extrasolar planets”, Virtual Meeting of the German Astronomical Society (2020)
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, ...