Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-03T13:44:31.112761Z
Paper Citation Record · LEDGER
Kilonova and progenitor properties of merger-driven gamma-ray bursts
As of 12 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2512.23354.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-26T00:49:47.927471Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
2 of 2 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved1
- parse uncertain0
- malformed identifier1
- metadata mismatch0
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
Observation 8b27ed9a-eace-4951-b0af-c11448d26117 · outbound
This paper cites Using Neural Networks to Perform Rapid High-Dimensional Kilonova Parameter Inference.
Kilonova and progenitor properties of merger-driven gamma-ray bursts Using Neural Networks to Perform Rapid High-Dimensional Kilonova Parameter Inference
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T13:44:31.001986Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 39672342-9cac-455a-b786-06ab85f61f4c · outbound
This paper cites In the case of the Top-Hat (TH) jet structure,θ w is not a model parameter andΦis fixed=30 (deg) for all NSBH models (see Section 3).
Kilonova and progenitor properties of merger-driven gamma-ray bursts In the case of the Top-Hat (TH) jet structure,θ w is not a model parameter andΦis fixed=30 (deg) for all NSBH models (see Section 3)
Reference 2
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-03T13:44:31.112761Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation 9614d35a-4a0d-4c8b-9012-236cce890faa · inbound
Nuclear Isomers and Their Impact on Gamma-Ray Emission in Binary Neutron Star Mergers cites this paper.
Nuclear Isomers and Their Impact on Gamma-Ray Emission in Binary Neutron Star Mergers Kilonova and progenitor properties of merger-driven gamma-ray bursts
Reference 41
- Resolution
- verified exact
- arxiv_id, observed 2026-07-30T02:04:28.573056Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.