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Paper Citation Record · LEDGER

Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1604.01022.

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

pith.paper-citation-record.v1
1604.01022 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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T14:34:28.350426Z

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

102
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation ed400bae-07f4-489a-a6a5-6a92b9996d56 · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:28.350426Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:28.350426Z digest=sha256:6b22a7aa5771cf0b329f52c6e865e9e776f71ecc22f9eb98e5bbb515f633d456

Observation 76024ee1-6a1a-4466-9459-382f6cc891f1 · inbound

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

Can current models predict the local black hole merger rate? Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries

Reference 178

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.673607Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6bd4d8b5e908495cba8302a6b1cc8d024b256aa7885309a879f4ef0d380499b9