activity
20112026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 6.2k across the 76 of their papers we have counts for

collaborators

76 papers

astro-ph.HE2026

ENGRAVE follow-up of a type IIb supernova spatially coincident with the sub-threshold gravitational wave trigger S250818k

K. Ackley, M. T. Botticella, A. Boye +54

The candidate gravitational wave (GW) event S250818k was one of only three non-retracted LIGO-Virgo-KAGRA public alerts issued during the fourth observing run of the network (O4) w…

astro-ph.HE2024

Binary neutron star merger offsets from their host galaxies. GW 170817 as a case study

N. Gaspari, H. F. Stevance, A. J. Levan +2

Aims. The locations of binary neutron star (BNS) mergers within their host galaxies encode the systemic kicks that these systems received in the supernova aftermath. We investigate…

astro-ph.GA2023

Recovering lost light: discovery of supernova remnants with integral field spectroscopy

Héctor Martínez-Rodríguez, Lluís Galbany, Carles Badenes +8

We present results from a systematic search for broad ( 400 \kms) \ha\ emission in Integral Field Spectroscopy data cubes of 1200 nearby galaxies obtained with PMAS and…

astro-ph.GA2023

A Machine Learning Approach to Galactic Emission-Line Region Classification

Carter Lee Rhea, Laurie Rousseau-Nepton, Ismael Moumen +13

Diagnostic diagrams of emission-line ratios have been used extensively to categorize extragalactic emission regions; however, these diagnostics are occasionally at odds with each o…

astro-ph.HE2023★ 1 cited

Environmental dependence of Type IIn supernova properties

Takashi J. Moriya, Lluis Galbany, Cristina Jimenez-Palau +9

Type IIn supernovae occur when stellar explosions are surrounded by dense hydrogen-rich circumstellar matter. The dense circumstellar matter is likely formed by extreme mass loss f…

astro-ph.SR2023★ 14 cited

A metallicity dependence on the occurrence of core-collapse supernovae

Thallis Pessi, Joseph P. Anderson, Joseph D. Lyman +5

Core-collapse supernovae (CCSNe) are widely accepted to be caused by the explosive death of massive stars with initial masses M. There is, however, a comparative…