Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
In-situ formation of star clusters at z > 7 via galactic disk fragmentation; shedding light on ultra-compact clusters and overmassive black holes seen by JWST
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2411.00670.
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 2026-08-09T18:37:35.991455Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-09T18:37:36.273511Z
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 6887a5cc-908d-4201-a89f-7c597fbbca2d · inbound
Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field cites this paper.
Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field In-situ formation of star clusters at z > 7 via galactic disk fragmentation; shedding light on ultra-compact clusters and overmassive black holes seen by JWST
Reference 36
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-09T18:37:36.279283Z
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 a5cae4bd-d4d3-4ec9-98e9-94aa08ec0782 · inbound
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity In-situ formation of star clusters at z > 7 via galactic disk fragmentation; shedding light on ultra-compact clusters and overmassive black holes seen by JWST
Reference 157
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:56.696776Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.