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Paper Citation Record · LEDGER

Production of Light Element Primary Process nuclei in neutrino-driven winds

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1007.1275.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1007.1275 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T14:23:02.395927Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T05:33:19.194031Z

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 719e1753-e355-47c8-a4bd-cdbb890a7282 · inbound

Metal-Poor Stars in the Milky Way System cites this paper.

Metal-Poor Stars in the Milky Way System Production of Light Element Primary Process nuclei in neutrino-driven winds

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-12T14:23:02.395927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T14:23:02.395927Z digest=sha256:72733f80c9eeb41c2b19a2c225d312bed2a1ceb037a49049abb093fd3eb41075

Observation 77c5b38f-57ca-4a66-99bc-aa9a89c94025 · inbound

Bayesian Analysis of the $^{86}$Sr$(\alpha, \alpha)$ Reaction to Constrain the $^{86}$Sr$(\alpha, n)$ Cross Section at Astrophysical Energies cites this paper.

Bayesian Analysis of the $^{86}$Sr$(\alpha, \alpha)$ Reaction to Constrain the $^{86}$Sr$(\alpha, n)$ Cross Section at Astrophysical Energies Production of Light Element Primary Process nuclei in neutrino-driven winds

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-08-05T05:33:19.198928Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-05T05:33:18.836761Z digest=sha256:f009ebdd23160ebb5a60e99f0d3e4ba7387cb458a5694fd00a92d60beb65e5fb