Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Reanalyze the pulsar scenario to explain the cosmic positron excess considering the recent developments
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1906.08542.
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 2026-05-24T06:48:57.946124Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-24T06:49:01.908093Z
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 96f879fd-6df5-4608-8ec1-52769f82cbbc · inbound
Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo cites this paper.
Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo Reanalyze the pulsar scenario to explain the cosmic positron excess considering the recent developments
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T06:49:01.911140Z
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 63e146a2-c24d-4be9-9b64-c2f926fbc945 · inbound
PHECT: A lightweight computation tool for pulsar halo emission cites this paper.
PHECT: A lightweight computation tool for pulsar halo emission Reanalyze the pulsar scenario to explain the cosmic positron excess considering the recent developments
Reference 27
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T23:02:52.281845Z
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.