Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Stellar feedback efficiencies: supernovae versus stellar winds
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1511.05151.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T15:55:28.488956Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-28T11:22:02.888525Z
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 7f22cd7b-e07a-4f94-ad82-f9c90dd5fb43 · inbound
Centrally concentrated star formation in young clusters II: Jet feedback cites this paper.
Centrally concentrated star formation in young clusters II: Jet feedback Stellar feedback efficiencies: supernovae versus stellar winds
Reference 72
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T11:22:02.889871Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 668885e2-ac17-403c-97c7-99b29e3fccb8 · inbound
FRANZ: Framework for analytical one-zone blastwave dynamics cites this paper.
FRANZ: Framework for analytical one-zone blastwave dynamics Stellar feedback efficiencies: supernovae versus stellar winds
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T11:43:18.801290Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5b867feb-972c-4f71-96ba-851899ea4b62 · inbound
Per Astronomix ad Astra: High-Order Differentiable (Magneto)hydrodynamics with Energy-Conserving Self-Gravity cites this paper.
Per Astronomix ad Astra: High-Order Differentiable (Magneto)hydrodynamics with Energy-Conserving Self-Gravity Stellar feedback efficiencies: supernovae versus stellar winds
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T15:55:28.488956Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.