Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Isolated Black Holes as Potential PeVatrons and Ultrahigh-energy Gamma-ray Sources
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2412.08136.
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 2026-08-07T22:27:46.953239Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T00:05:50.393231Z
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 f89b0d11-031b-4742-9f8a-0a50d58a75b4 · inbound
Galactic Isolated Stellar-Mass Black Holes with the Magnetospheric Spark Gap as Possible GeV-TeV Gamma-ray Unidentified Sources cites this paper.
Galactic Isolated Stellar-Mass Black Holes with the Magnetospheric Spark Gap as Possible GeV-TeV Gamma-ray Unidentified Sources Isolated Black Holes as Potential PeVatrons and Ultrahigh-energy Gamma-ray Sources
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T22:27:46.953239Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation adeddcb5-5817-4e3a-9124-e584e0475142 · inbound
How many VHE gamma-ray binaries with young pulsars can be observed? cites this paper.
How many VHE gamma-ray binaries with young pulsars can be observed? Isolated Black Holes as Potential PeVatrons and Ultrahigh-energy Gamma-ray Sources
Reference 9
- Resolution
- malformed identifier
- arxiv_id, observed 2026-05-11T00:05:50.395163Z
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.