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Erratum: “Self-consistent 3D Radiative Transfer for Kilonovae: Directional Spectra from Merger Simulations” (2023, ApJL, 954, L41)
Shingles, L. J. (Corresponding author)GSI* ; Collins, C. ; Vijayan, V.GSI* ; Flörs, A.GSI* ; Just, O.GSI* ; Leck, G.GSI* ; Xiong, Z.GSI* ; Bauswein, A.GSI* ; Martínez-Pinedo, G.GSI* ; Sim, S. A.
2025
Institute of Physics Publ.
London
Please use a persistent id in citations: doi:10.3847/2041-8213/ade719
Note: Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.
Contributing Institute(s):
- Nukleare Astrophysik & Struktur (KNA)
Research Program(s):
- KILONOVA - Probing r-process nucleosynthesis through its electromagnetic signatures (885281) (885281)
- GreatMoves - General Relativistic Moving-Mesh Simulations of Neutron-Star Mergers (759253) (759253)
- DFG project 279384907 - SFB 1245: Atomkerne: Von fundamentalen Wechselwirkungen zu Struktur und Sternen (279384907) (279384907)
- DFG project 138713538 - SFB 881: Das Milchstraßensystem (138713538) (138713538)
- DFG project 491382106 - Open-Access-Publikationskosten / 2022-2024 / GSI Helmholtzzentrum für Schwerionenforschung (491382106) (491382106)
- 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)
Experiment(s):
- no experiment theory work (theory)
Appears in the scientific report
2025
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