Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-03T09:20:43.799796Z
Paper Citation Record · LEDGER
Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars
As of 12 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 1 inbound Pith citation observation for arXiv:2601.14370.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T17:38:11.852003Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
2 of 2 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved1
- parse uncertain1
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation d3101d67-86df-4cff-a445-3780178d9f34 · outbound
This paper cites R., Iliev I.
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T09:20:43.755095Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eda5ff74-e9ec-45d7-bf8d-1c64455dd228 · outbound
This paper cites an unresolved cited work.
Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars Unresolved cited work
Reference 5
- Resolution
- parse uncertain
- no resolver link, observed 2026-08-03T09:20:43.799796Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation 7b0971e0-88a5-4f49-8171-7c5a01684fd5 · inbound
How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background cites this paper.
How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T17:38:11.852003Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.