Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A nebular origin for the persistent radio emission of fast radio bursts
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2312.15296.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-08T20:23:00.738577Z
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
4
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation e22e24b0-607f-4f04-9b82-5e9fe7ea2136 · inbound
A bright wideband radio burst from the isolated neutron star 2XMM J104608.7$-$594306 cites this paper.
A bright wideband radio burst from the isolated neutron star 2XMM J104608.7$-$594306 A nebular origin for the persistent radio emission of fast radio bursts
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T18:55:08.102908Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 5d50b57d-5a9e-42e2-92da-b655376339c0 · inbound
Signatures of Two Distinct Epochs of FRB 20240114A from January to August 2024 Based on its Energy and Waiting Time Analysis cites this paper.
Signatures of Two Distinct Epochs of FRB 20240114A from January to August 2024 Based on its Energy and Waiting Time Analysis A nebular origin for the persistent radio emission of fast radio bursts
Reference 207
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T08:27:47.816168Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation fe1683cf-3264-48a0-81b1-d903f95e6a17 · inbound
Unveiling the Local Environment of FRB 20220912A: Sub-arcsecond $4-26$ GHz Radio Continuum Mapping cites this paper.
Unveiling the Local Environment of FRB 20220912A: Sub-arcsecond $4-26$ GHz Radio Continuum Mapping A nebular origin for the persistent radio emission of fast radio bursts
Reference 13
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-08T20:25:37.258903Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.