Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the astrophysical robustness of neutron star merger r-process
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1206.2379.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:35:56.552674Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T16:16:43.721590Z
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 9856484a-21cf-4f7b-87aa-fe159ccad55a · 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 On the astrophysical robustness of neutron star merger r-process
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T11:35:56.552674Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 60555343-4a6f-498e-80d7-8f1bc8886b9c · inbound
Direct Measurement of the Accretion Disk Formed in Prompt Collapse Mergers with Future Gravitational-Wave Observatories cites this paper.
Direct Measurement of the Accretion Disk Formed in Prompt Collapse Mergers with Future Gravitational-Wave Observatories On the astrophysical robustness of neutron star merger r-process
Reference 35
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T16:16:43.726776Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 13f4dd18-26c7-438d-9e2c-327f46695587 · 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 On the astrophysical robustness of neutron star merger r-process
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:55:42.633317Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation caf2eaec-847a-4df9-9c6a-08da3169a2f9 · 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 On the astrophysical robustness of neutron star merger r-process
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T04:20:55.798518Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.