activity
20182022
most citedThe Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

40 citations · 112 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2022★ 12 cited

iPTF14hls in the circumstellar medium interaction model: A promising candidate for a pulsational pair-instability supernova

Ling-Jun Wang, Liang-Duan Liu, Wei-Li Lin +4

iPTF14hls is a luminous Type II supernova (SN) with a bumpy light curve that remains debated for its origin. It maintains roughly a constant effective temperature and luminosity si…

astro-ph.HE2021

SN 2015bf: a fast declining type II supernova with flash-ionised signatures

Han Lin, Xiaofeng Wang, Jujia Zhang +19

We present optical and ultraviolet photometry, as well as optical spectra, for the type II supernova (SN) 2015bf. Our observations cover the phases from to d af…

astro-ph.HE2021★ 19 cited

Supernova luminosity powered by magnetar-disk system

Weili Lin, Xiaofeng Wang, Lingjun Wang +1

Magnetars are one of the potential power sources for some energetic supernova explosions such as type I superluminous supernovae (SLSNe I) and broad-lined type Ic supernovae (SNe I…

astro-ph.HE2021★ 40 cited

The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

Danfeng Xiang, Xiaofeng Wang, Weili Lin +47

We present our photometric and spectroscopic observations on the peculiar transient AT2018cow. The multi-band photometry covers from peak to 70 days and the spectroscopy rang…

astro-ph.IM2020★ 36 cited

The Tsinghua University-Ma Huateng Telescopes for Survey: Overview and Performance of the System

Ji-Cheng Zhang, Xiao-Feng Wang, Jun Mo +16

Over the past decade, time-domain astronomy in optical bands has developed rapidly with the operations of some wide-field survey facilities. However, most of these surveys are cond…

astro-ph.HE2018★ 5 cited

A Pulsar Wind Nebula Model Applied to Short GRB 050724

Wei-Li Lin, Ling-Jun Wang, Zi-Gao Dai

A subset of short gamma-ray bursts (sGRBs) have been found to be characterized by near-infrared/optical bumps at days, some of which exhibit almost concurrent X-ray flares…