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Paper Citation Record · LEDGER

Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collision

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2204.03493.

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

pith.paper-citation-record.v1
2204.03493 v5

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 2026-08-07T06:34:17.273281+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: pith, observed 2026-07-08T17:55:20.713078Z

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 39cc01ce-1cbb-4ea8-ba34-92bbea51645d · 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 Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collision

Reference 190

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=sha256:788abd171248d6133b0738d54a4fd631b1b7fec0a0d68899931a40b29cda4d61

Observation c148be7c-31f1-434c-a012-fc9e7a7af6b5 · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap Formation of black holes in the pair-instability mass gap: Hydrodynamical simulations of a head-on massive star collision

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-07-08T17:55:20.714347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-07-08T17:53:06.845093Z digest=sha256:611d349067e53a05896bf2a8287df24c1d70d176f363c955db04e381b3bc7b5c