Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1612.04829.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:35:56.357644Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T09:26:51.308804Z
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 481fbc75-3362-438d-a344-48d409703982 · inbound
Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.
Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T11:35:56.357644Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation be39a38d-aac7-4563-8a48-bf8d14fa1b07 · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
Reference 44
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T09:26:51.310375Z
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 642b1df7-7f3c-4167-b605-6c5848ce02cc · inbound
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries cites this paper.
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:15:31.206535Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1b322d29-3fc9-4b19-b962-b9187b630abb · 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 Dynamics, nucleosynthesis, and kilonova signature of black hole - neutron star merger ejecta
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:55:43.512498Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.