Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Formation of the First Quasars. I. The Black Hole Seeds, Accretion and Feedback Models
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2012.01458.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T20:32:19.171955Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-08T20:32:20.486526Z
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 8f941d66-c46a-4e5b-9b57-8a6fa6c17e2e · inbound
A prevalent population of normal-mass central black holes in high-redshift massive galaxies cites this paper.
A prevalent population of normal-mass central black holes in high-redshift massive galaxies The Formation of the First Quasars. I. The Black Hole Seeds, Accretion and Feedback Models
Reference 45
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-08T20:32:20.491753Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 19a9df41-b0a8-4f2c-9a24-564af62c8283 · inbound
Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.
Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ The Formation of the First Quasars. I. The Black Hole Seeds, Accretion and Feedback Models
Reference 193
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T06:58:51.524418Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.