Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1807.09073.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T12:45:48.260261Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-29T03:33:06.478876Z
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 b2e6e1a4-b8d6-4ca4-87ea-ad4c38665874 · inbound
Comprehensive Variability Analysis of Blazars Using Fermi Light Curves Across Multiple Timescales cites this paper.
Comprehensive Variability Analysis of Blazars Using Fermi Light Curves Across Multiple Timescales The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T12:45:48.260261Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 92a5774c-3aed-4d35-a629-1be88f6c52ad · inbound
A Rare Gamma-ray Flaring episode of the Narrow-Line Seyfert 1 Galaxy 1H 0323+342 cites this paper.
A Rare Gamma-ray Flaring episode of the Narrow-Line Seyfert 1 Galaxy 1H 0323+342 The flux distribution of individual blazars as a key to understand the dynamics of particle acceleration
Reference 101
- Resolution
- verified exact
- local_arxiv, observed 2026-06-29T03:33:06.480224Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.