activity
20152023
most citedThe Most Luminous Supernova ASASSN-15lh: Signature of a Newborn Rapidly-Rotating Strange Quark Star

68 citations · 191 across the 6 of their papers we have counts for

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astro-ph.HE2023★ 18 cited

Reanalysis of the X-ray burst associated FRB 200428 with Insight-HXMT observations

M. Y. Ge, C. Z. Liu, S. N. Zhang +15

A double-peak X-ray burst from the Galactic magnetar SGR J1935+2154 was discovered as associated with the two radio pulses of FRB 200428 separated by 28.97+-0.02 ms. Precise measur…

astro-ph.HE2020★ 18 cited

Discovery of state transition behaviors in PSR J1124--5916

M. Y. Ge, J. P. Yuan, F. J. Lu +7

With the twelve-year long observations by {\sl Fermi}-LAT, we discover two pairs of spin-down state transitions of PSR J1124--5916, making it the second young pulsar detected to ha…

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…

astro-ph.HE2015★ 68 cited

The Most Luminous Supernova ASASSN-15lh: Signature of a Newborn Rapidly-Rotating Strange Quark Star

Z. G. Dai, S. Q. Wang, J. S. Wang +2

In this paper we show that the most luminous supernova discovered very recently, ASASSN-15lh, could have been powered by a newborn ultra-strongly-magnetized pulsar, which initially…