Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2407.09949.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T22:08:18.663533Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T11:36:57.494572Z
Reference resolution
0 of 0 outbound references displayed
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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 6af748a9-284d-4c86-b9f0-11d8f749c9aa · inbound
The Origin of Supermassive Black Holes from Pop III.1 Seeds cites this paper.
The Origin of Supermassive Black Holes from Pop III.1 Seeds The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T01:02:14.024755Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2c1fbe7d-956d-4677-a93d-870e4b22784c · inbound
Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr cites this paper.
Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T21:08:51.920479Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 49968df3-df0e-46aa-ad2d-6658a07d8a8e · inbound
Supermassive black hole growth in hierarchically merging nuclear star clusters cites this paper.
Supermassive black hole growth in hierarchically merging nuclear star clusters The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T11:36:57.502615Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation 42f614d4-f780-404c-8437-fab544a5475b · inbound
Robust {\mu}-distortion constraints on primordial supermassive black holes from cubic (gNL) non-Gaussian perturbations cites this paper.
Robust {\mu}-distortion constraints on primordial supermassive black holes from cubic (gNL) non-Gaussian perturbations The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T22:08:18.663533Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3eb83f39-28ab-40b5-bdc8-e740151d9ed4 · inbound
The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth cites this paper.
The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth The formation of supermassive black holes from Population III.1 seeds. III. Galaxy evolution and black hole growth from semi-analytic modelling
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T08:41:19.122141Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.