Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2106.09909.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T19:19:19.420059Z
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
30
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation d41754a0-bbbb-47c1-be0c-5c841d313a9d · inbound
Impact of rotation on the accretion of entropy perturbations in collapsing massive stars cites this paper.
Impact of rotation on the accretion of entropy perturbations in collapsing massive stars A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T19:19:19.420059Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 61dad06a-3f63-477a-a40d-51cc26d53746 · inbound
Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors cites this paper.
Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors A three-dimensional hydrodynamics simulation of oxygen-shell burning in the final evolution of a fast-rotating massive star
Reference 204
- Resolution
- verified exact
- local_arxiv, observed 2026-07-11T00:07:39.503476Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.