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Ish: A Comparison of Three Neodymium Atomic Data Sets for Kilonova Modeling
[CLC][ITAL]r[/ITAL][/CLC]-Process in Neutron Star Mergers
C. Freiburghaus, Stephan Rosswog, F.‐K. Thielemann
Maqola19996 iqtibosABIA kilonova as the electromagnetic counterpart to a gravitational-wave source
Stephen Smartt, T. W. Chen, Anders Jerkstrand +97
Maqola20175 iqtibosABIOn the astrophysical robustness of the neutron star merger r-process
O. Korobkin, S. Rosswog, A. Arcones +1
Maqola20125 iqtibosABISystematic opacity calculations for kilonovae
Masaomi Tanaka, Daiji Kato, Gediminas Gaigalas +1
Maqola20204 iqtibosABINLTE effects on kilonova expansion opacities
Quentin Pognan, Anders Jerkstrand, Jon Grumer
Maqola20224 iqtibosABIThe X-ray counterpart to the gravitational-wave event GW170817
E. Troja, L. Piro, Hendrik van Eerten +31
Maqola20173 iqtibosABIIdentification of strontium in the merger of two neutron stars
D. Watson, C. J. Hansen, J. Selsing +15
Maqola20193 iqtibosABINebular Emission from Lanthanide-rich Ejecta of Neutron Star Merger
Kenta Hotokezaka, Masaomi Tanaka, Daiji Kato +1
Maqola20213 iqtibosABIOn the validity of steady-state for nebular phase kilonovae
Quentin Pognan, Anders Jerkstrand, Jon Grumer
Maqola20213 iqtibosABI