activity
20132025
most citedNLTE Effects on Kilonova Expansion Opacities

57 citations · 380 across the 18 of their papers we have counts for

collaborators

18 papers

physics.atom-ph2025★ 2 cited

multiconfigurational calculations of experimentally significant energy levels and transition rates in Lr I

Joseph S. Andrews, Andrey I. Bondarev, Per Jönsson +4

Large-scale multiconfigurational calculations are conducted on experimentally significant transitions in Lr I and its lanthanide homologue Lu I, exhibiting good agreement with rece…

astro-ph.HE2024★ 12 cited

Actinide signatures in low electron fraction kilonova ejecta

Quentin Pognan, Meng-Ru Wu, Gabriel Martínez-Pinedo +4

Neutron star (NS) mergers are known to produce heavy elements through rapid neutron capture (r-process) nucleosynthesis. Actinides are expected to be created solely by the r-proces…

physics.atom-ph2024★ 2 cited

Targeted optimization in small-scale atomic structure calculations: application to Au I

Sema Caliskan, Jon Grumer, Anish M. Amarsi

The lack of reliable atomic data can be a severe limitation in astrophysical modelling, in particular of events such as kilonovae that require information on all neutron-capture el…

astro-ph.HE2023★ 41 cited

NLTE Spectra of Kilonovae

Quentin Pognan, Jon Grumer, Anders Jerkstrand +1

The electromagnetic transient following a binary neutron star merger is known as a kilonova (KN). Owing to rapid expansion velocities and small ejecta masses, KNe rapidly transitio…

astro-ph.SR2023★ 13 cited

Extended atomic data for oxygen abundance analyses

W. Li, P. Jönsson, A. M. Amarsi +2

As the most abundant element in the universe after hydrogen and helium, oxygen plays a key role in planetary, stellar, and galactic astrophysics. Its abundance is especially influe…

physics.atom-ph2023★ 10 cited

Extended MCDHF calculations of energy levels and transition data for N I

Meichun Li, Wenxian Li, P. Jönsson +2

Accurate and extensive atomic data are essential for spectroscopic analyses of stellar atmospheres and other astronomical objects. We present energy levels, lifetimes, and transiti…