孙新翔
|
|
My research focuses on Gamma-Ray Bursts (GRBs), electromagnetic counterparts of gravitational waves, and fast X-ray transients. I am particularly interested in the outcomes of binary neutron star (BNS) mergers, the maximum mass of neutron stars, and the classification and physical mechanisms of high-energy transients.
2024~Present National Astronomical Observatories, CAS PhD Student
2020.8~2024.6 College of Physics, Jilin University Bachelor of Science
2026.3 - present teaching assistant of the postgraduate course High Energy Astrophysics at the University of Chinese Academy of Sciences
2025.9 - present transient advocate(TA) of the Einstein Probe
2025 Pulsar Summer School (August 1–10, 2025, Beijing) Outstanding Student
2024.10~2025.6 Operator of UCAS70 telescope, responsible for observation execution, daily operations, routine maintenance, and troubleshooting.
2. Qiang Xi, Ning-Chen Sun, David Aguado, Ismael Pérez-Fournon, Frédérick Poidevin, Junjie Jin, Yiming Mao, Zexi Niu, Beichuan Wang, Yu Zhang et al. SN 2024aecx: A Fast-evolving Type IIb Supernova with a Prominent Shock-cooling Peak, The Astrophysical Journal, DOI: 10.3847/1538-4357/ae2d06
1.Liu, Mingjun; Zhang, Yijia; Wang, Yun; Xue, Rui; Buckley, David; Howell, D. Andrew; Jin, Chichuan; Li, Wenxiong; Monageng, Itumeleng; Pan, Haiwu et al. Detection of an Orphan X-Ray Flare from a Blazar Candidate EP240709a with the Einstein Probe, The Astrophysical Journal, DOI: 10.3847/1538-4357/adc301
