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Paper Citation Record · LEDGER

Large-Scale Structure with Gravitational Waves I: Galaxy Clustering

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1205.1512.

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

pith.paper-citation-record.v1
1205.1512 v2

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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

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

50
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation c3fef83b-efd0-40cb-90e4-180f9632b0f3 · inbound

Sensitivity of Weak Lensing Surveys to Gravitational Waves from Inspiraling Supermassive Black Hole Binaries cites this paper.

Sensitivity of Weak Lensing Surveys to Gravitational Waves from Inspiraling Supermassive Black Hole Binaries Large-Scale Structure with Gravitational Waves I: Galaxy Clustering

Reference 36

Resolution
verified exact
local_arxiv, observed 2026-05-16T19:28:19.746017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:667e1d98660b54544f40433c9a1181dea9c992e6059369ac3d2f0dcfd4eceb5c

Observation db9cebdf-eff5-4cc6-b978-5b4ee7d0b31f · inbound

Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias cites this paper.

Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias Large-Scale Structure with Gravitational Waves I: Galaxy Clustering

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-05-09T06:40:42.994998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-08T18:11:52.949061Z digest=sha256:8ef8e4dd6478086d78cc1e2b68aa35d97a07cac7e1112e46d68d764fa1e83522