Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
3D radiative transfer kilonova modelling for binary neutron star merger simulations
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2209.05246.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:55.927562Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-19T04:37:04.171871Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation f1d00be1-2272-42ab-a112-34d96dd66950 · inbound
Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities cites this paper.
Calibrated Lanthanide Atomic Data for Kilonova Radiative Transfer. I. Atomic Structure and Opacities 3D radiative transfer kilonova modelling for binary neutron star merger simulations
Reference 197
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:41:19.370572Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 95896f37-8abf-4025-91cd-1b90f07610ff · inbound
R-process heating implementation in hydrodynamic simulations with neural networks cites this paper.
R-process heating implementation in hydrodynamic simulations with neural networks 3D radiative transfer kilonova modelling for binary neutron star merger simulations
Reference 85
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T04:37:04.175291Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation 1411b15b-b5a7-4c2b-8f66-dc5888e46953 · inbound
Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers cites this paper.
Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers 3D radiative transfer kilonova modelling for binary neutron star merger simulations
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T08:41:25.562066Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation 5b9d7026-6c24-4b85-89d9-f0d8c2c2f960 · inbound
Late-time emission-line profiles from kilonova models cites this paper.
Late-time emission-line profiles from kilonova models 3D radiative transfer kilonova modelling for binary neutron star merger simulations
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T09:02:10.553457Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ffdbf183-b821-4f12-8754-020f5d15ee89 · inbound
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures 3D radiative transfer kilonova modelling for binary neutron star merger simulations
Reference 121
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:55:48.109632Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 833c3326-3ce9-430a-a633-0db8f6353f61 · inbound
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves cites this paper.
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves 3D radiative transfer kilonova modelling for binary neutron star merger simulations
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T04:20:55.927562Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.