Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Astrophysical S factor of {$^{12}$C($\alpha,\gamma$)$^{16}$O} Calculated with the Reduced R-matrix Theory
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1509.00725.
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 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 83d93a96-a821-4fe2-92df-bc49bcefd0f4 · inbound
Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars cites this paper.
Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars Astrophysical S factor of {$^{12}$C($\alpha,\gamma$)$^{16}$O} Calculated with the Reduced R-matrix Theory
Reference 54
- Resolution
- verified exact
- doi, observed 2026-05-09T02:16:32.060235Z
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.