activity
20172024
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 1.1k across the 10 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE2024

The fast transient AT 2023clx in the nearby LINER galaxy NGC 3799 as a tidal disruption of a very low-mass star

P. Charalampopoulos, R. Kotak, T. Wevers +30

We present an extensive analysis of the optical and UV properties of AT2023clx, the closest TDE to date, that occurred in the nucleus of the interacting LINER galaxy, NGC3799 (z=0.…

astro-ph.HE2023

SN 2021gno: a Calcium-rich transient with double-peaked light curves

K. Ertini, G. Folatelli, L. Martinez +52

We present extensive ultraviolet (UV) and optical photometric and optical spectroscopic follow-up of supernova (SN)~2021gno by the "Precision Observations of Infant Supernova Explo…

astro-ph.HE202248 cited

A persistent ultraviolet outflow from an accreting neutron star binary transient

N. Castro Segura, C. Knigge, K. S. Long +31

All disc-accreting astrophysical objects produce powerful outflows. In binaries containing neutron stars (NS) or black holes, accretion often takes place during violent outbursts.…

astro-ph.HE2021

PISCOLA: a data-driven transient light-curve fitter

Tomás E. Müller-Bravo, Mark Sullivan, Mathew Smith +4

Forthcoming time-domain surveys, such as the Rubin Observatory Legacy Survey of Space and Time, will vastly increase samples of supernovae (SNe) and other optical transients, requi…

astro-ph.HE20219 cited

Transitional events in the spectrophotometric regime between stripped envelope and superluminous supernovae

S. J. Prentice, C. Inserra, S. Schulze +24

The division between stripped-envelope supernovae (SE-SNe) and superluminous supernovae (SLSNe) is not well defined in either photometric or spectroscopic space. While a sharp lumi…

astro-ph.HE20215 cited

SN 2019hcc: A Type II Supernova Displaying Early O II Lines

Eleonora Parrag, Cosimo Inserra, Steve Schulze +18

We present optical spectroscopy together with ultraviolet, optical and near-infrared photometry of SN 2019hcc, which resides in a host galaxy at redshift 0.044, displaying a sub-so…