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Paper Citation Record · LEDGER

The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1204.1043.

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

pith.paper-citation-record.v1
1204.1043 v2

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 2026-08-05T06:32:48.257954+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-05-24T08:53:31.777812Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-24T08:54:15.785878Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 35deb553-46ed-45f5-b536-c8a583c81f68 · inbound

Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter cites this paper.

Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries

Reference 17

Resolution
verified exact
local_arxiv, observed 2026-05-24T08:54:15.788477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-24T08:53:31.777812Z digest=sha256:1c3710102cfc0d56333ca640f75e615df1cea4be68b2abbe8c66d13387f6b348

Observation 4c6c94a4-2aed-4c28-a4ea-43733983e0da · inbound

Gravitational waveform from radial infall at the third-and-half Post-Newtonian order cites this paper.

Gravitational waveform from radial infall at the third-and-half Post-Newtonian order The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-05-12T01:41:20.138632Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-12T01:40:05.664304Z digest=sha256:cf3aa9848ea853472c2f7b0b301b2159bbc63f44bb8c30c00e3623ba8599310d

Observation 2e518248-8694-410f-a2b5-64f4898430c5 · inbound

Convergence of post-Newtonian for quasi-circular non-precessing comparable mass ratios BBHs cites this paper.

Convergence of post-Newtonian for quasi-circular non-precessing comparable mass ratios BBHs The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-05-21T06:24:00.587439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-21T06:22:04.929858Z digest=sha256:9a06ad68cbd790aa4dcf6165d50c5846d5eb5d4227242e7d69ce72c83eae9d03