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Paper Citation Record · LEDGER

Signatures of R-process Enrichment in Supernovae from Collapsars

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2205.10421.

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

pith.paper-citation-record.v1
2205.10421 v1

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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:10:39.355904Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T00:43:40.075910Z

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 712b61e0-fbcd-4431-8e37-6dec124e139a · inbound

Ultraheavy Ultrahigh-Energy Cosmic Rays cites this paper.

Ultraheavy Ultrahigh-Energy Cosmic Rays Signatures of R-process Enrichment in Supernovae from Collapsars

Reference 50

Resolution
verified exact
arxiv_id, observed 2026-05-24T00:43:40.078848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-24T00:42:49.655371Z digest=sha256:e2b801751f82928aa10c453e017c743afbd1572413f0822edc0dae9bc49ebedb

Observation 187dc790-77bc-4d58-98b4-c9ef57c196b4 · inbound

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos cites this paper.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Signatures of R-process Enrichment in Supernovae from Collapsars

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-15T19:10:39.355904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T19:10:39.355904Z digest=sha256:a47bd0e2cd2e99ef96f030ed8b07e4d6e7816ed8011120e4ef045a03434563f7