Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Powerful explosions from the collapse of rotating supermassive stars
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2408.11572.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T11:53:33.027266Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T12:16:16.480190Z
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 8156bcf3-f039-474e-8160-a4d154755618 · inbound
Formation of supermassive stars and dense star clusters in metal-poor clouds exposed to strong FUV radiation cites this paper.
Formation of supermassive stars and dense star clusters in metal-poor clouds exposed to strong FUV radiation Powerful explosions from the collapse of rotating supermassive stars
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T11:58:34.690347Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation f8d8b4c3-2e67-4170-8fe4-c9b23bd9d0ef · inbound
SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement cites this paper.
SACRA-2D: New axisymmetric general relativistic hydrodynamics code with fixed mesh refinement Powerful explosions from the collapse of rotating supermassive stars
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T05:33:08.058157Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.