Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Multi-wavelength study of a hyperluminous X-ray source near NGC 6099: a strong IMBH candidate
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2503.00904.
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 2026-08-06T17:38:27.378291Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T09:21:20.806149Z
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 a8467a1d-cfc1-42d9-a1a5-7dbdd5004e7e · inbound
The Complex Multi-Wavelength Morphology of the Peculiar Compact Galaxy Group IC 2431 cites this paper.
The Complex Multi-Wavelength Morphology of the Peculiar Compact Galaxy Group IC 2431 Multi-wavelength study of a hyperluminous X-ray source near NGC 6099: a strong IMBH candidate
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T17:38:27.378291Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a82f3c70-bd19-467d-9d26-8f151f7b255e · inbound
Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.
Predicting intermediate-mass black hole formation in star clusters with machine learning Multi-wavelength study of a hyperluminous X-ray source near NGC 6099: a strong IMBH candidate
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T09:21:20.808546Z
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.