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Paper Citation Record · LEDGER

Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2102.01689.

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

pith.paper-citation-record.v1
2102.01689 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:02:46.179263Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T01:02:56.187239Z

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 2fc2b02f-e7c8-466f-8e1d-12faa21a6125 · inbound

Dissecting environmental effects with eccentric gravitational wave sources cites this paper.

Dissecting environmental effects with eccentric gravitational wave sources Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-07T05:02:46.179263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:02:46.179263Z digest=sha256:41dafbf7ed742a742e5f516bd0730150b60e12748fe16f3ca95d35a6a0215049

Observation 739e6976-dd51-42d4-8007-449871615e20 · inbound

Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework cites this paper.

Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events

Reference 59

Resolution
verified exact
arxiv_id, observed 2026-06-29T01:02:56.188650Z

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=pdf_text observed=2026-06-29T00:58:22.089350Z digest=sha256:eb91b74b01132b27074ecb78df7119758e78fbf458761d3deffd6a631e021a2d

Observation 4e7dcc62-414c-4ef9-a63a-d7ee781d0a72 · inbound

Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits cites this paper.

Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events

Reference 76

Resolution
unresolved
no resolver link, observed 2026-07-13T01:31:57.131208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T01:31:57.131208Z digest=sha256:a66ec9c68e7d2933a32d062be62c7239850c31f52c06035c33ce07830f9bfc31

Observation 6b83ab51-d3b2-4307-810b-9e0baa24e068 · inbound

Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits cites this paper.

Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-02T07:36:10.771371Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T07:36:10.771371Z digest=sha256:29ff88e21de1130d0a0bbbd5f9141fb5d6fe9d4706b1187b91bdddce378aadd5