Paper Citation Record · LEDGER

3D radiative transfer kilonova modelling for binary neutron star merger simulations

As of 15 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.

pith.paper-citation-record.v1
2209.05246 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:20:55.927562Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-19T04:37:04.171871Z

Reference resolution

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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 2026-08-15T06:32:42.880941+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 2026-08-15T06:32:42.880941+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.