Pan, J.-S.; Ting, Y.-S.; Yu, J.: Astroconformer: The prospects of analysing stellar light curves with transformer-based deep learning models. Monthly Notices of the Royal Astronomical Society 528, pp. 5890 - 5903 (2024)
Yu, J.; Khanna, S.; Themessl, N.; Hekker, S.; Dréau, G.; Gizon, L.; Bi, S.: Revised Extinctions and Radii for 1.5 Million Stars Observed by APOGEE, GALAH, and RAVE. The Astrophysical Journal Supplement Series 264, p. 41 (2023)
Borre, C. C.; Aguirre Børsen-Koch, V.; Helmi, A.; Koppelman, H. H.; Nielsen, M. B.; Rørsted, J. L.; Stello, D.; Stokholm, A.; Winther, M. L.; Davies, G. R.et al.; Hon, M.; Kruijssen, J. M. D.; Laporte, C. F. P.; Reyes, C.; Yu, J.: Age determination of galaxy merger remnant stars using asteroseismology. Monthly Notices of the Royal Astronomical Society 514, pp. 2527 - 2544 (2022)
Borre, C. C.; Aguirre Børsen-Koch, V.; Helmi, A.; Koppelman, H. H.; Nielsen, M. B.; Rørsted, J. L.; Stello, D.; Stokholm, A.; Winther, M. L.; Davies, G. R.et al.; Hon, M.; Kruijssen, J. M. D.; Laporte, C. F. P.; Reyes, C.; Yu, J.: Age determination of galaxy merger remnant stars using asteroseismology. Monthly Notices of the Royal Astronomical Society 514, pp. 2527 - 2544 (2022)
Dréau, G.; Lebreton, Y.; Mosser, B.; Bossini, D.; Yu, J.: Characterising the AGB bump and its potential to constrain mixing processes in stellar interiors. Astronomy and Astrophysics 668, p. A115 (2022)
Gehan, C.; Gaulme, P.; Yu, J.: Surface magnetism of rapidly rotating red giants: Single versus close binary stars. Astronomy and Astrophysics 668, p. A116 (2022)
Murphy, S. J.; Li, T.; Sekaran, S.; Bedding, T. R.; Yu, J.; Tkachenko, A.; Colman, I.; Huber, D.; Hey, D.; Baratashvili, T.et al.; Janssens, S.: A binary with a δ Scuti star and an oscillating red giant: orbit and asteroseismology of KIC 9773821. Monthly Notices of the Royal Astronomical Society 505 (2), pp. 2336 - 2348 (2021)
Yu, J.; Hekker, S.; Bedding, T. R.; Stello, D.; Huber, D.; Gizon, L.; Khanna, S.; Bi, S.: Asteroseismology of luminous red giants with Kepler: II. Dependence of mass-loss on pulsations and radiation. Monthly Notices of the Royal Astronomical Society 501 (4), pp. 5135 - 5148 (2021)
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".