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Paper Citation Record · LEDGER

Two-Dimensional Simulations of Pulsational Pair-Instability Supernovae

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1402.4134.

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

pith.paper-citation-record.v1
1402.4134 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:24:14.491628Z

measured 1 of 1 external citation measurements

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

77
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 981be363-d21c-4f5d-895b-34098c125855 · inbound

Origins of Supermassive Black Holes in Galactic Centers cites this paper.

Origins of Supermassive Black Holes in Galactic Centers Two-Dimensional Simulations of Pulsational Pair-Instability Supernovae

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-07T14:24:14.491628Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:24:14.491628Z digest=sha256:d067da6aa31cc47251de4e1cf6e0e51f169ed0e26b00cf3d1cdfc09201022375

Observation 9f59108e-c8a7-4b48-bea5-2a362ecdb41c · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? Two-Dimensional Simulations of Pulsational Pair-Instability Supernovae

Reference 82

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.754429Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:25e8aecb57c95dc305e633857dc88825eb412b55632c0431129f00c64dc032af