Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Magnetic Driving of Relativistic Outflows in Active Galactic Nuclei. I. Interpretation of Parsec-Scale Accelerations
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0310747.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:39.528530Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-24T04:33:53.828732Z
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 61e6b12b-4817-4597-9b8d-7dc1bc82a4ea · inbound
A closer look at the electromagnetic signatures of Bethe-Heitler pair production process in blazars cites this paper.
A closer look at the electromagnetic signatures of Bethe-Heitler pair production process in blazars Magnetic Driving of Relativistic Outflows in Active Galactic Nuclei. I. Interpretation of Parsec-Scale Accelerations
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-05-24T04:33:53.832610Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 4f60b77f-b469-49c5-87a0-ffcfbb117fc7 · inbound
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Magnetic Driving of Relativistic Outflows in Active Galactic Nuclei. I. Interpretation of Parsec-Scale Accelerations
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T17:19:39.528530Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.