Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Radio to Gamma-Ray Emission from Shell-type Supernova Remnants: Predictions from Non-linear Shock Acceleration Models
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9810158.
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 2026-07-14T05:16:35.864642Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-19T22:17:49.148862Z
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 48b1da51-e70e-4809-b6b2-119f9665650b · inbound
Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87 cites this paper.
Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87 Radio to Gamma-Ray Emission from Shell-type Supernova Remnants: Predictions from Non-linear Shock Acceleration Models
Reference 67
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T22:17:49.150357Z
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 10f4c023-b93d-4c5f-884d-b4adc34f54f0 · inbound
Superdiffusion of cosmic rays in the vicinity of their accelerators and the resulting $\gamma$-ray emission cites this paper.
Superdiffusion of cosmic rays in the vicinity of their accelerators and the resulting $\gamma$-ray emission Radio to Gamma-Ray Emission from Shell-type Supernova Remnants: Predictions from Non-linear Shock Acceleration Models
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T05:16:35.864642Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.