Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Solar type III radio burst time characteristics at LOFAR frequencies and the implications for electron beam transport
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1802.01507.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
34
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 5a80330b-5ecf-4a99-86ae-fedd668e06d4 · inbound
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona cites this paper.
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona Solar type III radio burst time characteristics at LOFAR frequencies and the implications for electron beam transport
Reference 40
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-25T03:06:33.688256Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation f62667d2-04af-4463-8f41-97ce4516de01 · inbound
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona cites this paper.
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona Solar type III radio burst time characteristics at LOFAR frequencies and the implications for electron beam transport
Reference 40
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-30T15:14:46.461282Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.