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Paper Citation Record · LEDGER

Implications of massive close binaries for black hole formation and supernovae

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/9904256.

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

pith.paper-citation-record.v1
astro-ph/9904256 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T19:09:31.860525Z

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

18
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d680842a-02f5-49b5-a031-d3491ab5b8d4 · inbound

Physics-driven Explosions of Stripped High-Mass Stars: Synthetic Light Curves and Spectra of Stripped-Envelope Supernovae with Broad Lightcurves cites this paper.

Physics-driven Explosions of Stripped High-Mass Stars: Synthetic Light Curves and Spectra of Stripped-Envelope Supernovae with Broad Lightcurves Implications of massive close binaries for black hole formation and supernovae

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-12T19:09:31.860525Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T19:09:31.860525Z digest=sha256:16d4c0116afbb9e49b1575c3778d57c2ac1dc83167d63587433d3f233524a493

Observation 964a6af9-78c3-4946-827b-06ed28a52d78 · inbound

Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae cites this paper.

Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae Implications of massive close binaries for black hole formation and supernovae

Reference 187

Resolution
metadata mismatch
arxiv_id, observed 2026-05-13T17:55:46.398479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-09T20:40:25.240969Z digest=sha256:42df099a4474c07ef934489cf3dc6e6622748786ecc43a0a5089e5efaa1b970d

Observation 31c7bb1e-5e7f-46af-b059-c967a8814ba5 · inbound

Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae cites this paper.

Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae Implications of massive close binaries for black hole formation and supernovae

Reference 187

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T22:10:10.018291Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-07-04T22:05:18.893335Z digest=sha256:23ec3331f91197d0ce99d45b39365cc523449e938ca5b18cb4208936dc1e1b9b

Observation eecca6eb-cbd5-459b-979e-d78699913b3d · inbound

Type Ib supernovae are bluer than Type Ic supernovae cites this paper.

Type Ib supernovae are bluer than Type Ic supernovae Implications of massive close binaries for black hole formation and supernovae

Reference 239

Resolution
verified exact
arxiv_id, observed 2026-05-13T17:55:46.398479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-05-09T19:09:55.718148Z digest=sha256:42e78be173b68f64290ade980cb1fe7ce1b74c3fd114df930783169ef10020c7

Observation 5c7f4586-7859-490b-ac01-41b0a0462747 · inbound

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models Implications of massive close binaries for black hole formation and supernovae

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.376498Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:f10363d9b267a0c3dde2e24bd5fabc57e4131238c20af658e8924cc27d1dcb3f

Observation 012e8772-3d03-4ce9-a7fd-554d317990c8 · inbound

SN 2023rve: A Type II Supernova with No Nebular Oxygen cites this paper.

SN 2023rve: A Type II Supernova with No Nebular Oxygen Implications of massive close binaries for black hole formation and supernovae

Reference 107

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:05:12.034850Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-01T01:04:17.215743Z digest=sha256:55daaab7d9e4367c51d74c55ca3122baa742a48f89b7092408a3435d8f6b0def