Paper Citation Record · LEDGER

Probing the large scale structure using gravitational-wave observations of binary black holes

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2005.01111.

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

pith.paper-citation-record.v1
2005.01111 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 2026-08-06T06:34:29.942622+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-26T20:15:37.780290Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T01:39:25.063349Z

Reference resolution

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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 3a112fcd-d80b-4bb7-ab90-28ccd1aea8b4 · inbound

Constraining the lensing dispersion from the angular clustering of binary black hole mergers cites this paper.

Constraining the lensing dispersion from the angular clustering of binary black hole mergers Probing the large scale structure using gravitational-wave observations of binary black holes

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-19T10:17:15.978159Z

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.

Observation 91cea72a-bc11-437b-b9bd-e13cac5057e0 · inbound

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies cites this paper.

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies Probing the large scale structure using gravitational-wave observations of binary black holes

Reference 121

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.469019Z

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.

Observation e9eb04ff-17ec-42c5-97b4-9ff1c5a22532 · inbound

A unified harmonic framework for dark siren cosmology cites this paper.

A unified harmonic framework for dark siren cosmology Probing the large scale structure using gravitational-wave observations of binary black holes

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:30:31.183604Z

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.

Observation 431ce909-3129-47b0-b203-c6ff8f796260 · inbound

Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters cites this paper.

Impact of the Einstein Telescope's duty cycle on the estimation of binary black holes parameters Probing the large scale structure using gravitational-wave observations of binary black holes

Reference 100

Resolution: verified exact; arxiv_id, observed 2026-07-04T01:39:25.065731Z

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.