Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Heavy Black Hole Seed Formation in High-z Atomic Cooling Halos
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2312.06769.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T22:49:13.697433Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-18T12:11:22.870457Z
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 aeadb2a7-3770-4957-ae93-3f32bbf56788 · inbound
Direct Collapse Black Hole Candidates from Decaying Dark Matter cites this paper.
Direct Collapse Black Hole Candidates from Decaying Dark Matter Heavy Black Hole Seed Formation in High-z Atomic Cooling Halos
Reference 5
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T12:11:22.873016Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 6a52c5e6-187c-4021-8674-a1fbcca13aca · inbound
A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales cites this paper.
A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales Heavy Black Hole Seed Formation in High-z Atomic Cooling Halos
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T22:50:26.225211Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 669cbc5f-33c4-486a-906f-e249a2a3926d · inbound
A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales cites this paper.
A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales Heavy Black Hole Seed Formation in High-z Atomic Cooling Halos
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T22:49:13.697433Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.