activity
20182026
most citedProbing the Shock Breakout Signal of SN 2024ggi from the Transformation of Early Flash Spectroscopy

29 citations · 145 across the 23 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2023★ 10 cited

Minute-cadence Observations of the LAMOST Fields with the TMTS: III. Statistic Study of the Flare Stars from the First Two Years

Qichun Liu, Jie Lin, Xiaofeng Wang +22

Tsinghua University-Ma Huateng Telescopes for Survey (TMTS) aims to detect fast-evolving transients in the Universe, which has led to the discovery of thousands of short-period var…

astro-ph.SR2022★ 18 cited

An 18.9-minute Blue Large-Amplitude Pulsator Crossing the 'Hertzsprung Gap' of Hot Subdwarfs

Jie Lin, Chengyuan Wu, Xiaofeng Wang +28

Blue large-amplitude pulsators (BLAPs) represent a new and rare class of hot pulsating stars with unusually large amplitudes and short periods. Up to now, only 24 confirmed BLAPs h…

astro-ph.SR2022★ 10 cited

Simultaneous Detection of Optical Flares of the Magnetically Active M Dwarf Wolf 359

Han-Tang Lin, Wen-Ping Chen, Jinzhong Liu +13

We present detections of stellar flares of Wolf\,359, an M6.5 dwarf in the solar neighborhood (2.41~pc) known to be prone to flares due to surface magnetic activity. The observatio…

astro-ph.SR2020★ 25 cited

Can Helium-detonation Model Explain the Observed Diversity of Type Ia Supernovae?

Wenxiong Li, Xiaofeng Wang, Mattia Bulla +13

We study a sample of 16 Type Ia supernovae (SNe Ia) having both spectroscopic and photometric observations within 2 3 days after the first light. The early colors of such…

astro-ph.SR2018★ 5 cited

SN 2014J in M82: New Insights On the Spectral Diversity of Type Ia Supernovae

Kaicheng Zhang, Xiaofeng Wang, JuJia Zhang +25

We present extensive spectroscopic observations for one of the closest type Ia supernovae (SNe Ia), SN 2014J discovered in M82, ranging from 10.4 days before to 473.2 days after B-…