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Paper Citation Record · LEDGER

Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/0205122.

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

pith.paper-citation-record.v1
gr-qc/0205122 v3

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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:31:50.125565Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-13T00:25:44.142471Z

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 3aaa9f50-9b52-4e74-8295-41838adf957e · inbound

Post-Newtonian Theory for Gravitational Waves cites this paper.

Post-Newtonian Theory for Gravitational Waves Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case

Reference 108

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:09:17.158904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-05-13T00:25:43.700226Z digest=sha256:ae4aef52a5f5ba93103b8d1d9cdacb02527a3c0568f2c363b093581a2d467719

Observation cdbdcd98-5c66-4265-b790-530ac13bf6ec · inbound

Innermost stable circular orbit of arbitrary-mass compact binaries at fourth post-Newtonian order cites this paper.

Innermost stable circular orbit of arbitrary-mass compact binaries at fourth post-Newtonian order Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-16T04:31:50.125565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:31:50.125565Z digest=sha256:2b475d19b753673031e3ebba94649b9cbbe4c1e9c97756bb9f6d4ddd89a2e00d