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Paper Citation Record · LEDGER

Progenitor Model of SN 1987A Based on the Slow Merger Scenario

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1705.04084.

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

pith.paper-citation-record.v1
1705.04084 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T06:51:42.465920Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T12:10:23.139865Z

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 a9eb36ab-6586-4e18-8892-5cecfe78b2e8 · inbound

Rotation-induced Relaxation of Supernova Constraints on Axionlike Particles cites this paper.

Rotation-induced Relaxation of Supernova Constraints on Axionlike Particles Progenitor Model of SN 1987A Based on the Slow Merger Scenario

Reference 53

Resolution
verified exact
arxiv_id, observed 2026-07-04T22:24:23.246963Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-10T04:37:19.629956Z digest=sha256:a933bfbdeefbfa5048cdc9acf72c002e78902007a1b42db5e2197d92c4d63461

Observation dab1aa9a-2760-42ec-85de-5394a9834f59 · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins Progenitor Model of SN 1987A Based on the Slow Merger Scenario

Reference 36

Resolution
unresolved
no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:19a956fed67157e9a8027b037d194a216a67e07b1f79b41f07e1b4eaf9f558a6