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Paper Citation Record · LEDGER

Accurate time-domain gravitational waveforms for extreme-mass-ratio binaries

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:gr-qc/0609002.

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

pith.paper-citation-record.v1
gr-qc/0609002 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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:42:40.199750Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T00:42:47.790107Z

Reference resolution

0 of 0 outbound references displayed

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  • malformed identifier0
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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 2bbc8a0f-a228-4b6c-a6c8-a2ace7e07167 · inbound

Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries cites this paper.

Consistency of spin effects between numerical relativity and perturbation theory for inspiraling comparable-mass black hole binaries Accurate time-domain gravitational waveforms for extreme-mass-ratio binaries

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-04T13:28:15.145063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T13:28:15.145063Z digest=sha256:8d2c509483d8bdc3d42e2e6778bbc0fd497071578fc193b8196a5f1b57171d17

Observation 6e21d3df-6c68-4344-91ff-59b7daf3a192 · inbound

Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications cites this paper.

Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications Accurate time-domain gravitational waveforms for extreme-mass-ratio binaries

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-03T22:13:54.319355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T22:13:54.319355Z digest=sha256:b6b90c98eaebd1948652aefddc4a3b0c33e0dab9af69f202632e3a75b8a4d15a

Observation 9993ecf6-fced-4a41-bac4-c9586bd61820 · inbound

Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers cites this paper.

Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers Accurate time-domain gravitational waveforms for extreme-mass-ratio binaries

Reference 107

Resolution
verified exact
local_arxiv, observed 2026-08-06T00:42:47.869710Z

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=2026-08-06T00:42:40.199750Z digest=sha256:3eaee477476d565f948e666908c09168caffdad89015641a5190fd3554bee8dd