Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Simulating the formation of massive seed black holes in the early Universe. I: An improved chemical model
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1501.05960.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T19:03:20.465418Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
3
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 12f0c5c9-1ad6-46d5-8d59-80589563edbe · inbound
Little Red reionization factories cites this paper.
Little Red reionization factories Simulating the formation of massive seed black holes in the early Universe. I: An improved chemical model
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T19:03:20.465418Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 475efaac-809e-48f8-8ed4-d1409ef48fd0 · inbound
Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages cites this paper.
Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages Simulating the formation of massive seed black holes in the early Universe. I: An improved chemical model
Reference 191
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T21:52:40.320634Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation e046ad13-9168-4fbf-b608-e2558dc8bad7 · inbound
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations Simulating the formation of massive seed black holes in the early Universe. I: An improved chemical model
Reference 92
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T04:20:32.629387Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.