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Cited article:

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Simple Model for Temporal Variations of Hα Spectrum by an Eruptive Filament from a Superflare on a Solar-type Star

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Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic Environment

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High-velocity Blue-shifted Fe xxv Heα Line during a Superflare of the RS Canum Venaticorum–type Star IM Peg

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Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data

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Evolution of brightness and magnetic features of young solar-type stars – II. The young F8 star HIP 71933

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Active longitudes and starspot evolution of the young rapidly rotating star USNO-B1.0 1388−0463685 discovered in the Yunnan–Hong Kong survey

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Topological changes in the magnetic field of LQ Hya during an activity minimum

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Investigation on Doppler Imaging and Chromospheric Activity of the Young Dwarf LQ Hya Based on High-resolution Spectroscopy

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Probable detection of an eruptive filament from a superflare on a solar-type star

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Astronomy & Astrophysics 646 A6 (2021)
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Stellar coronal mass ejections – II. Constraints from spectroscopic observations

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Monthly Notices of the Royal Astronomical Society 494 (3) 3766 (2020)
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A Likely Magnetic Activity Cycle for the Exoplanet Host M Dwarf GJ 3512

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Starspot evolution, differential rotation, and correlation between chromospheric and photospheric activities on Kepler-411

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Spot evolution on LQ Hya from 2006–2017: temperature maps based on SOFIN and FIES data

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