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 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations 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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:33:23.014179Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T11:33:23.842807Z
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 bed194a7-f699-4ba1-9259-71af346ab9fb · inbound
Background in $\gamma$-ray detectors and carbon beam tests in the Felsenkeller shallow-underground accelerator laboratory cites this paper.
Background in $\gamma$-ray detectors and carbon beam tests in the Felsenkeller shallow-underground accelerator laboratory Astrophysical S factor of {$^{12}$C($\alpha,\gamma$)$^{16}$O} Calculated with the Reduced R-matrix Theory
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T11:33:23.928719Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
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 2026-08-18T06:34:40.430872+00:00.