Silvotti, R.; Schuh, S.; Kim, S.-L.; Lutz, R.; Reed, M.; Benatti, S.; Janulis, R.; Lanteri, L.; Østensen, R.; Marsh, T. R.et al.; Dhillon, V. S.; Paparo, M.; Molnar, L.: The sdB pulsating star V391 Peg and its putative giant planet revisited after 13 years of time-series photometric data. Astronomy and Astrophysics 611, A85 (2018)
Silvotti, R.; Charpinet, S.; Green, E.; Fontaine, G.; Telting, J. H.; Østensen, R. H.; Van Grootel, V.; Baran, A. S.; Schuh, S.; Fox Machado, L.: Kepler detection of a new extreme planetary system orbiting the subdwarf-B pulsator KIC 10001893. Astronomy and Astrophysics 570, A130 (2014)
Adamczak, J.; Werner, K.; Rauch, T.; Schuh, S.; Drake, J. J.; Kruk, J. W.: Chandra grating spectroscopy of three hot white dwarfs. Astronomy and Astrophysics 546, A1 (2012)
Lehmann, H.; Zechmeister, M.; Dreizler, S.; Schuh, S.; Kanzler, R.: KIC 4247791: a SB4 system with two eclipsing binaries (2EBs) A quadruple system? Astronomy and Astrophysics 541, A105 (2012)
Schuh, S.; Silvotti, R.; Lutz, R.; Kim, S.-L.; The Exotime Collaboration Team: The EXOTIME monitoring program discovers substellar companion candidates around the rapidly pulsating subdwarf B stars V1636 Ori and DW Lyn. Astronomical Society of the Pacific Conference Series 481, pp. 5 - 11 (2014)
Mackebrandt, F.; Schuh, S.; Silvotti, R.: The EXOTIME project: Using the stellar pulsation timing method to detect sub-stellar companions. Virtual Annual Meeting of the Astronomische Gesellschaft 2020
(2020)
Mackebrandt, F.; Schuh, S.; Silvotti, R.: The stellar pulsation timing method to detect substellar companions. Annual Meeting of the Astronomische Gesellschaft 2017 , Splinter HotStars, Göttingen, Germany (2017)
Schuh, S.: Stellar pulsation timing - A complementary science case for the PLATO mission. Planetary Systems Beyond The Main Sequence II, Technion, Haifa, Israel (2017)
Schuh, S.; Silvotti, R.: The O-C diagram of V391 Peg revisited: planet or not? The many Scales of the Universe: Galaxies, their Suns, and their Planets Annual Meeting of the Astronomische Gesellschaft 2017 , Göttingen, Germany (2017)
Schuh, S.: Stellar pulsation and the search for new worlds. Royal Astronomical Society Specialist Discussion - Asteroseismoloy: high-precision stellar metrics for the exoplanet era, London, UK (2015)
Mackebrandt, F.; Schuh, S.: The stellar pulsation timing method to detect substellar companions. Planets Days Workshop, IAU General Assembly 2018, Vienna, Austria (2018)
Mackebrandt, F.; Schuh, S.: The stellar pulsation timing detection method for substellar companions. The PLATO Mission Conference 2017: Exoplanetary systems in the PLATO era, Warwick, UK (2017)
Mackebrandt, F.; Schuh, S.: The stellar pulsation timing detection method for substellar companions. Planetary Systems Beyond The Main Sequence II, Technion, Haifa, Israel (2017)
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.
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".