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Paper Citation Record · LEDGER

An upper limit on the spins of merging binary black holes formed through binary evolution

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2311.14041.

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

pith.paper-citation-record.v1
2311.14041 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T14:34:33.896643Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 594dacf8-105e-4bad-b4b0-758f91c14909 · 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 An upper limit on the spins of merging binary black holes formed through binary evolution

Reference 111

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:33.896643Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:33.896643Z digest=sha256:1beee2ccaf52e24c14aa32db7cfeae134f2de0c58d939e832448bbda9d1acb67

Observation 087abe88-3989-4f96-b5a5-4d80eeae3c43 · inbound

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

Can current models predict the local black hole merger rate? An upper limit on the spins of merging binary black holes formed through binary evolution

Reference 91

Resolution
metadata mismatch
arxiv_id, observed 2026-06-28T13:02:10.698657Z

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=arxiv_source observed=2026-06-28T13:01:54.102298Z digest=sha256:ec0c9e7a48e09571f21cad5a99833a713aa9aad6d014b1eacad51620a4e4a1b2

Observation 1af4b173-bfa5-43f6-b01f-540aaa258504 · inbound

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 cites this paper.

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 An upper limit on the spins of merging binary black holes formed through binary evolution

Reference 39

Resolution
verified exact
arxiv_id, observed 2026-07-03T12:58:07.818409Z

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=2026-06-27T08:41:37.044992Z digest=sha256:afe1cfcea611559f57492288afdd6b2fef580b322d32b5314650728243544e4f