activity
20242026
most citedElectron impact excitation of Te IV and V and Level Resolved R-matrix Photoionization of Te I - IV with application to modelling of AT2017gfo

1 citations · 1 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

Ce II-IV emission in kilonovae with R-matrix collision strengths and distorted wave recombination rates

Leo Patrick Mulholland, Niamh Ferguson, Luke J. Shingles +3

We provide transition probabilities and Maxwellian-averaged collision-strengths for the electron-impact excitation of Ce {\sc ii} - {\sc iv}. These ions are potentially abundant in…

astro-ph.HE2025★ 1 cited

Electron impact excitation of Te IV and V and Level Resolved R-matrix Photoionization of Te I - IV with application to modelling of AT2017gfo

Leo P. Mulholland, Catherine A. Ramsbottom, Connor P. Ballance +2

Spectral modelling of kilonovae (KNe) require large amounts of collisional excitation and photoionization atomic data for lowly ionised (neutral, singly and doubly ionised) species…

astro-ph.SR2025

New Level Resolved Ground and Excited State Pb III, IV, V & VI Photoionization Cross Sections for Heavy Metal Subdwarf Modeling

David J. Dougan, Matti Dorsch, Laura J. A. Scott +3

High abundances of various lead (Pb) species have been identified in the spectra of many Asymptotic Giant Branch (AGB) stars and O- and B-type subdwarfs (sdO/B). Additional atomic…

astro-ph.SR2025

Strontium I, III, IV and V: Electron Impact Excitation Data for Kilonovae and White Dwarf Diagnostic Applications

David J. Dougan, Niall E. McElroy, Connor P. Ballance +1

Strontium (Sr) emissions have been observed across a wide range of astrophysical phenomena, from kilonovae (KNe) events to white dwarf (WD) stars. Precise and extensive atomic data…

physics.atom-ph2025

Electron-Impact Excitation of Zirconium I-III in support of Neutron Star Merger Diagnostics

M. McCann, C. P. Ballance, F. McNeill +2

Recent observation and analysis of kilonovae (KNe) spectra as a result of neutron star mergers require accurate and complete atomic structure and collisional data for interpretatio…

astro-ph.HE2025

On the use of the Axelrod formula for thermal electron collisions in Astrophysical Modelling

Leo P. Mulholland, Steven J. Bromley, Connor P. Ballance +2

The Axelrod approximation is widely used in astrophysical modelling codes to evaluate electron-impact excitation effective collision strengths for forbidden transitions. Approximat…

astro-ph.SR2024

Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks

Leo Patrick Mulholland, Fiona McNeill, Stuart A. Sim +2

Tellurium is a primary candidate for the identification of the 2.1 m emission line in kilonovae (KNe) spectra AT2017gfo and GRB230307A. Despite this, there is currently an insuf…