Education & Employments：

B.S. in astronomy, School of Astronomy and Space Science, Nanjing University, 2009.09-2013.06.

Ph.D. in astronomy, School of Astronomy and Space Science, Nanjing University, 2013.09-2018.06.

Postdoctoral research fellow and assistant researcher, Department of Physics, Tsinghua University, 2018.09-2024.02.

Associate professor, Department of Astronomy, Xiamen University, since 2024.03.

Reseach interests：

Observations and theories of supernovae and gamma-ray bursts.

Publications：

Lin, W. L., et al., A superluminous supernova lightened by collisions with pulsational pair-instability shells. Nature Astronomy, 7, 779 (2023).

Wang, X. F., Lin, W. L., et al., ASASSN-14ms: the Most Energetic Explosion of A Type Ibn Supernova and Its Physical Origin, The Astrophysical Journal, 917, 97 (2021).

Lin, W. L., et al., Supernova luminosity powered by magnetar-disk system, The Astrophysical Journal Letters, 914, L2 (2021).

Lin, W. L., et al., A Unified Accreting Magnetar Model for Long-duration Gamma-Ray Bursts and Some Stripped-envelope Supernovae, The Astrophysical Journal Letters, 903, L24 (2020).

Lin, W. L., et al., SN 2018hti: a nearby superluminous supernova discovered in a metal-poor galaxy, Monthly Notices of the Royal Astronomical Society, 497, 318 (2020).

Lin, W. L., et al., A Pulsar Wind Nebula Model Applied to Short GRB 050724, The Astrophysical Journal, 855, 67 (2018).

Lin, W. L. & Dai, Z. G., Estimate of an environmental magnetic field of fast radio bursts, Research in Astronomy and Astrophysics, 16, 38 (2016).