activity
20132026
most citedObservation of a charged charmoniumlike structure in at GeV

297 citations · 3.8k across the 84 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2025★ 3 cited

An extremely soft and weak fast X-ray transient associated with a luminous supernova

W. -X. Li, Z. -P. Zhu, X. -Z. Zou +101

Long gamma-ray bursts (LGRBs), including their subclasses of low-luminosity GRBs (LL-GRBs) and X-ray flashes (XRFs) characterized by low spectral peak energies, are known to be ass…

astro-ph.HE2024★ 30 cited

A fast X-ray transient from a weak relativistic jet associated with a type Ic-BL supernova

H. Sun, W. -X. Li, L. -D. Liu +163

Massive stars end their lives as core-collapse supernovae, amongst which some extremes are broad-lined type Ic supernovae from Wolf-Rayet stars associated with long-duration gamma-…

astro-ph.HE2017★ 27 cited

Broad-lined type Ic supernova iPTF16asu: A challenge to all popular models

L. J. Wang, X. F. Wang, Z. Cano +9

It is well-known that ordinary supernovae (SNe) are powered by 56Ni cascade decay. Broad-lined type Ic SNe (SNe Ic-BL) are a subclass of SNe that are not all exclusively powered by…

astro-ph.HE2017★ 12 cited

A Monte Carlo approach to magnetar-powered transients: II. Broad-lined type Ic supernovae not associated with GRBs

Ling-Jun Wang, Zach Cano, Shan-Qin Wang +11

Broad-lined type Ic supernovae (SNe Ic-BL) are a subclass of rare core collapse SNe whose energy source is debated in the literature. Recently a series of investigations on SNe Ic-…

astro-ph.HE2016★ 30 cited

Evidence for magnetar formation in broad-lined type Ic supernovae 1998bw and 2002ap

L. J. Wang, H. Yu, L. D. Liu +6

Broad-lined type Ic supernovae (SNe Ic-BL) are peculiar stellar explosions that distinguish themselves from ordinary SNe. Some SNe Ic-BL are associated with long-duration (\gtrsim…

astro-ph.HE2015★ 45 cited

A Triple-Energy-Source Model for Superluminous Supernova iPTF13ehe

S. Q. Wang, L. D. Liu, Z. G. Dai +2

Almost all superluminous supernovae (SLSNe) whose peak magnitudes are mag can be explained by the Ni-powered model, magnetar-powered (highly magnetized pulsar…