activity
20172023
most citedAn elliptical accretion disk following the tidal disruption event AT 2020zso

48 citations · 409 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2023★ 6 cited

Hidden shock powering the peak of SN 2020faa

I. Salmaso, E. Cappellaro, L. Tartaglia +9

The link between the fate of the most massive stars and the resulting supernova (SN) explosion is still a matter of debate, in major part because of the ambiguity among light-curve…

astro-ph.HE2023★ 42 cited

The optical light curve of GRB 221009A: the afterglow and the emerging supernova

M. D. Fulton, S. J. Smartt, L. Rhodes +46

We present extensive optical photometry of the afterglow of GRB~221009A. Our data cover \,days from the time of \textit{Swift} and \textit{Fermi} GRB detections. Photom…

astro-ph.HE2022★ 6 cited

Early Lightcurves of Type Ia Supernovae are Consistent with Nondegenerate Progenitor Companions

J. Burke, D. A. Howell, D. J. Sand +16

If Type Ia supernovae (SNe~Ia) result from a white dwarf being ignited by Roche lobe overflow from a nondegenerate companion, then as the supernova explosion runs into the companio…

astro-ph.HE2022★ 21 cited

SN2020qlb: A hydrogen-poor superluminous supernova with well-characterized light curve undulations

S. L. West, R. Lunnan, C. M. B. Omand +21

SN\,2020qlb (ZTF20abobpcb) is a hydrogen-poor superluminous supernova (SLSN-I) that is among the most luminous (maximum M mag) and that has one of the longest rise t…

astro-ph.HE2022★ 48 cited

An elliptical accretion disk following the tidal disruption event AT 2020zso

T. Wevers, M. Nicholl, M. Guolo +25

[Abridged] We classify AT 2020zso as a TDE based on the blackbody evolution inferred from UV/optical photometric observations, and spectral line content and evolution. We identify…

astro-ph.HE2022★ 21 cited

A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run

J. Rastinejad, K. Paterson, W. Fong +9

We present a comprehensive analysis of 653 optical candidate counterparts reported during the third gravitational wave (GW) observing run. Our sample concentrates on candidates fro…