most citedA very luminous jet from the disruption of a star by a massive black hole

131 citations · 152 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2022131 cited

A very luminous jet from the disruption of a star by a massive black hole

Igor Andreoni, Michael W. Coughlin, Daniel A. Perley +78

Tidal disruption events (TDEs) are bursts of electromagnetic energy released when supermassive black holes (SMBHs) at the centers of galaxies violently disrupt a star that passes t…

astro-ph.HE202214 cited

The Interaction of Supernova 2018evt with a Substantial Amount of Circumstellar Matter -- An SN1997cy-like Event

Yi Yang, Dietrich Baade, Peter Hoeflich +29

A rare class of supernovae (SNe) is characterized by strong interaction between the ejecta and several solar masses of circumstellar matter (CSM) as evidenced by strong Balmer-line…

astro-ph.HE2022

A search for relativistic ejecta in a sample of ZTF broad-lined Type Ic supernovae

Alessandra Corsi, Anna Y. Q. Ho, S. Bradley Cenko +23

The dividing line between gamma-ray bursts (GRBs) and ordinary stripped-envelope core-collapse supernovae (SNe) is yet to be fully understood. Observationally mapping the variety o…

astro-ph.HE2022

The Search for a Counterpart to NuSTAR J053449+2126.0

Antonio C. Rodriguez, Yuhan Yao, Kishalay De +1

Tumer et al. 2022, ATel #15171, have recently reported the discovery of an X-ray source, NuSTAR J053449+2126.0, during a calibration observation which took place on 25 April 2020.…

astro-ph.HE20227 cited

A Tight Three-parameter Correlation and Related Classification on Gamma-Ray Bursts

Shuai Zhang, Lang Shao, Bin-Bin Zhang +4

Gamma-ray bursts (GRBs) are widely believed to be from massive collapsars and/or compact binary mergers, which accordingly, would generate long and short GRBs, respectively. The de…

astro-ph.HE2020

ZTF Early Observations of Type Ia Supernovae II: First Light, the Initial Rise, and Time to Reach Maximum Brightness

A. A. Miller, Y. Yao, M. Bulla +17

While it is clear that Type Ia supernovae (SNe) are the result of thermonuclear explosions in C/O white dwarfs (WDs), a great deal remains uncertain about the binary companion that…