Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1610.08541.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T04:31:30.021909Z
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
114
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 6bcc01a2-e02f-473f-a660-24cf4c69c39a · inbound
Multidisciplinary Science in the Multimessenger Era cites this paper.
Multidisciplinary Science in the Multimessenger Era i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T04:31:30.021909Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 51550d46-1115-4e66-a4af-157db0930864 · inbound
Three Extremely Metal-Poor stars: discovery of a new CEMP-no star cites this paper.
Three Extremely Metal-Poor stars: discovery of a new CEMP-no star i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
Reference 220
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T06:41:43.668221Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 4f1cf881-1d00-451a-b063-ab535f131dfd · inbound
The impact of nuclear uncertainties on the p-process nucleosynthesis in Supernovae cites this paper.
The impact of nuclear uncertainties on the p-process nucleosynthesis in Supernovae i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs
Reference 290
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T04:41:01.740863Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.