Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Binary neutron star mergers as the source of the highest energy cosmic rays
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2405.12004.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T19:51:26.342186Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T11:39:46.736220Z
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 bdf2b9a6-0051-48bb-ae2e-e5e9c831257c · inbound
Ultraheavy Ultrahigh-Energy Cosmic Rays cites this paper.
Ultraheavy Ultrahigh-Energy Cosmic Rays Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 97
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T00:43:40.261577Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation daaf95dd-ac8a-4247-a655-4c2eff09c000 · inbound
The Global Cosmic Ray Observatory -- Challenging next-generation multi-messenger astronomy with interdisciplinary research cites this paper.
The Global Cosmic Ray Observatory -- Challenging next-generation multi-messenger astronomy with interdisciplinary research Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T19:51:26.342186Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 685808a0-6f39-4659-a38a-10a087fe0d7d · inbound
Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays cites this paper.
Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 15
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T23:55:31.191149Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation d75ccc90-b0f3-4cd2-af70-5c8480d45314 · inbound
A magnetar formation in binary neutron star merger cites this paper.
A magnetar formation in binary neutron star merger Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:37:45.132135Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation b5b0684c-1379-4f15-a27d-9597e9347050 · inbound
Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation cites this paper.
Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T11:39:46.737765Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 4ee005d9-d533-47ee-8a33-a886b8a71de6 · inbound
Ultra-High-Energy Particle Production in Binary Mergers Endowed with Magnetic Fields cites this paper.
Ultra-High-Energy Particle Production in Binary Mergers Endowed with Magnetic Fields Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:48:49.867444Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e85b41a1-8ff2-48c0-ae49-bd95fd313dbc · inbound
Proton-air interaction properties at $\sqrt{s} \simeq 100$ TeV from shower-depth measurements with the Pierre Auger Observatory and their connection to the Muon Puzzle cites this paper.
Proton-air interaction properties at $\sqrt{s} \simeq 100$ TeV from shower-depth measurements with the Pierre Auger Observatory and their connection to the Muon Puzzle Binary neutron star mergers as the source of the highest energy cosmic rays
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T05:12:26.591580Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.