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Large-scale atomic data calculations in Ce V – X ions for application to early kilonova emission from neutron star mergers

Monthly notices of the Royal Astronomical Society, 2022-02, Vol.509 (4), p.6138-6154

2022

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Calculation of forbidden transitions in doubly ionized neodymium (Nd III) of interest for kilonova nebular phase analysis

Journal of physics. B, Atomic, molecular, and optical physics, 2024-05, Vol.57 (10), p.105002

2024

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Multiconfiguration Dirac–Hartree–Fock radiative parameters for emission lines in Ce ii–iv ions and cerium opacity calculations for kilonovae

Monthly notices of the Royal Astronomical Society, 2021-02, Vol.501 (1), p.1440-1452

2021

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Atomic data and opacity calculations in La v–x ions for the investigation of kilonova emission spectra

Monthly notices of the Royal Astronomical Society, 2022-05, Vol.513 (2), p.2302-2325

2022

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Comparative study of kilonova opacities for three elements of the sixth period (hafnium, osmium, and gold) from new atomic structure calculations in Hf I–IV, Os I–IV, and Au I–IV

Astronomy and astrophysics (Berlin), 2024-07, Vol.687, p.A41

2024

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Opacity calculations in four to nine times ionized Pr, Nd, and Pm atoms for the spectral analysis of kilonovae

Monthly notices of the Royal Astronomical Society, 2023-01, Vol.518 (1), p.332-352

2023

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Overview of the contributions from all lanthanide elements to kilonova opacity in the temperature range from 25 000 to 40 000 K

Astronomy and astrophysics (Berlin), 2024-05, Vol.685, p.A91

2024

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Expansion and line-binned opacities of samarium ions for the analysis of early kilonova emission from neutron star mergers

Monthly notices of the Royal Astronomical Society, 2023-04, Vol.522 (1), p.312-318

2023

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Calculated oscillator strengths for the strongest lines of cosmochronological interest in the visible spectrum of singly ionized uranium (U II)

Monthly notices of the Royal Astronomical Society, 2018-11

2018

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Statistical RTA simulations of atomic data for astrophysical opacity modeling in the context of kilonova emission

Journal of physics. B, Atomic, molecular, and optical physics, 2024-02, Vol.57 (3), p.35001

2024

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Spectral line list of potential cosmochronological interest deduced from new calculations of radiative transition rates in singly ionized thorium (Th ii)

Monthly notices of the Royal Astronomical Society, 2020-08, Vol.496 (4), p.4507-4516

2020

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Plasma environment effects on K lines of astrophysical interest

Astronomy and astrophysics (Berlin), 2022-01, Vol.657

2022

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Opacities of singly and doubly ionized neodymium and uranium for kilonova emission modeling

Monthly notices of the Royal Astronomical Society, 2023-07, Vol.524 (2), p.3083-3101

2023

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Photoionization Models for High-density Gas

The Astrophysical journal, 2021-02, Vol.908 (1), p.94

2021

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Photoionization Modeling and the K Lines of Iron

The Astrophysical journal. Supplement series, 2004-12, Vol.155 (2), p.675-701

2004

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MCDHF calculations of isotope shifts of even-parity fine-structure levels in neutral osmium

Journal of quantitative spectroscopy & radiative transfer, 2016-12, Vol.185, p.70-78

2016

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Semi-empirical studies of atomic transition probabilities, oscillator strengths and radiative lifetimes in Hf II

Journal of quantitative spectroscopy & radiative transfer, 2015-09, Vol.163, p.39-49

2015

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PHOTOIONIZATION MODELING OF OXYGEN K ABSORPTION IN THE INTERSTELLAR MEDIUM: THE CHANDRA GRATING SPECTRA OF XTE J1817-330

The Astrophysical journal, 2013-05, Vol.768 (1), p.1-11

2013

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Oscillator strengths for high-excitation Ti ii from laboratory measurements and calculations

Monthly notices of the Royal Astronomical Society, 2016-07, Vol.460 (1), p.356-362

2016

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Updated opacities from the Opacity Project

Monthly notices of the Royal Astronomical Society, 2005-06, Vol.360 (2), p.458-464

2005

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A comparative study between semi-empirical oscillator strength parametrization and relativistic Hartree–Fock methods for computing the radiative parameters in Zr II spectrum

Journal of quantitative spectroscopy & radiative transfer, 2015-10, Vol.164, p.193-206

2015

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Lifetime measurements using two-step laser excitation for high-lying even-parity levels and improved theoretical oscillator strengths in Y ii

Monthly notices of the Royal Astronomical Society, 2017-01, Vol.471 (1), p.532-540

2017

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Experimental radiative lifetimes for highly excited states and calculated oscillator strengths for lines of astrophysical interest in singly ionized cobalt (Co ii)

Monthly notices of the Royal Astronomical Society, 2016-11, Vol.462 (4), p.3912-3917

2016

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Lifetime measurements and oscillator strengths in singly ionized scandium and the solar abundance of scandium

Monthly notices of the Royal Astronomical Society, 2017, Vol.472 (3), p.3337-3353

2017

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K-Shell Photoabsorption and Photoionisation of Trace Elements I. Isoelectronic Sequences With Electron Number 3< or = N < or = 11

Astronomy and astrophysics (Berlin), 2016-05, Vol.589, p.A137

2016

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Large-scale atomic data calculations in Ce V – X ions for application to early kilonova emission from neutron star mergers

Calculation of forbidden transitions in doubly ionized neodymium (Nd III) of interest for kilonova nebular phase analysis

Multiconfiguration Dirac–Hartree–Fock radiative parameters for emission lines in Ce ii–iv ions and cerium opacity calculations for kilonovae

Atomic data and opacity calculations in La v–x ions for the investigation of kilonova emission spectra

Comparative study of kilonova opacities for three elements of the sixth period (hafnium, osmium, and gold) from new atomic structure calculations in Hf I–IV, Os I–IV, and Au I–IV

Opacity calculations in four to nine times ionized Pr, Nd, and Pm atoms for the spectral analysis of kilonovae

Overview of the contributions from all lanthanide elements to kilonova opacity in the temperature range from 25 000 to 40 000 K

Expansion and line-binned opacities of samarium ions for the analysis of early kilonova emission from neutron star mergers

Calculated oscillator strengths for the strongest lines of cosmochronological interest in the visible spectrum of singly ionized uranium (U II)

Statistical RTA simulations of atomic data for astrophysical opacity modeling in the context of kilonova emission

Spectral line list of potential cosmochronological interest deduced from new calculations of radiative transition rates in singly ionized thorium (Th ii)

Plasma environment effects on K lines of astrophysical interest

Opacities of singly and doubly ionized neodymium and uranium for kilonova emission modeling

Photoionization Models for High-density Gas

Photoionization Modeling and the K Lines of Iron

MCDHF calculations of isotope shifts of even-parity fine-structure levels in neutral osmium

Semi-empirical studies of atomic transition probabilities, oscillator strengths and radiative lifetimes in Hf II

PHOTOIONIZATION MODELING OF OXYGEN K ABSORPTION IN THE INTERSTELLAR MEDIUM: THE CHANDRA GRATING SPECTRA OF XTE J1817-330

Oscillator strengths for high-excitation Ti ii from laboratory measurements and calculations

Updated opacities from the Opacity Project

A comparative study between semi-empirical oscillator strength parametrization and relativistic Hartree–Fock methods for computing the radiative parameters in Zr II spectrum

Lifetime measurements using two-step laser excitation for high-lying even-parity levels and improved theoretical oscillator strengths in Y ii

Experimental radiative lifetimes for highly excited states and calculated oscillator strengths for lines of astrophysical interest in singly ionized cobalt (Co ii)

Lifetime measurements and oscillator strengths in singly ionized scandium and the solar abundance of scandium

K-Shell Photoabsorption and Photoionisation of Trace Elements I. Isoelectronic Sequences With Electron Number 3< or = N < or = 11

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