Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
As of 31 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2407.01678.
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 2026-07-31T06:34:12.847434+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-28T09:30:56.846406Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T03:56:35.627562Z
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 79bbcfe6-72f7-4529-99dc-cea7f1df5f7d · inbound
Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence cites this paper.
Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
Reference 47
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T02:33:43.020828Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.
Observation 9e2a369a-0a07-4ad8-b490-aec678bc687e · inbound
3C403: a candidate neutrino-emitting radio galaxy cites this paper.
3C403: a candidate neutrino-emitting radio galaxy A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T07:52:09.393931Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.
Observation 6dd5314b-e195-42c5-8773-ed391eaf1283 · inbound
Single-source-class interpretation of the diffuse astrophysical neutrino flux cites this paper.
Single-source-class interpretation of the diffuse astrophysical neutrino flux A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
Reference 61
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T10:16:22.627632Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.
Observation e04b008a-ae67-423c-b9e6-f711fb97797d · inbound
Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes cites this paper.
Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
Reference 22
- Resolution
- verified exact
- arxiv_id, observed 2026-05-15T05:25:04.316128Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.
Observation 8ad93ddb-e2f1-45be-939c-528b5781e9ed · inbound
Probing Inelastic Dark Matter via Cosmic-Ray Upscattering in NGC 1068 cites this paper.
Probing Inelastic Dark Matter via Cosmic-Ray Upscattering in NGC 1068 A magnetized strongly turbulent corona as the source of neutrinos from NGC 1068
Reference 82
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-02T03:56:35.629054Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-31T06:34:12.847434+00:00.