activity
20152026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 3.3k across the 96 of their papers we have counts for

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Showing 2022Show all

7 papers · 1 filter

astro-ph.SR2022★ 17 cited

SN 2016dsg: A Thermonuclear Explosion Involving A Thick Helium Shell

Yize Dong, Stefano Valenti, Abigail Polin +29

A thermonuclear explosion triggered by a helium-shell detonation on a carbon-oxygen white dwarf core has been predicted to have strong UV line blanketing at early times due to the…

astro-ph.HE2022★ 36 cited

The nuclear transient AT 2017gge: a tidal disruption event in a dusty and gas-rich environment and the awakening of a dormant SMBH

F. Onori, G. Cannizzaro, P. G. Jonker +28

We present the results from a dense multi-wavelength (optical/UV, near-infrared (IR), and X-ray) follow-up campaign of the nuclear transient AT2017gge, covering a total of 1698 day…

astro-ph.HE2022

Euclid: Searching for pair-instability supernovae with the Deep Survey

T. J. Moriya, C. Inserra, M. Tanaka +106

Pair-instability supernovae are theorized supernovae that have not yet been observationally confirmed. They are predicted to exist in low-metallicity environments. Because overall…

astro-ph.HE2022★ 1 cited

Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja

Griffin Hosseinzadeh, Charles D. Kilpatrick, Yize Dong +56

We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby ( Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interactio…

astro-ph.HE2022

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

SN 2018bsz: a Type I superluminous supernova with aspherical circumstellar material

M. Pursiainen, G. Leloudas, E. Paraskeva +26

We present a spectroscopic analysis of Type I superluminous supernova (SLSN-I), SN 2018bsz. While it closely resembles SLSNe-I, the multi-component H line appearing at …