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)
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
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.