Paper Citation Record · LEDGER

Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1702.00872.

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

pith.paper-citation-record.v1
1702.00872 v2

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T16:30:11.450740Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T02:52:00.046332Z

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 6597514c-738a-49f7-a939-f1d3bc771a1b · inbound

Kicking gravitational wave detectors with recoiling black holes cites this paper.

Kicking gravitational wave detectors with recoiling black holes Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-14T13:50:47.400181Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 62be2990-011f-4524-8dd8-abf6a33ab161 · inbound

Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms cites this paper.

Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-09T11:24:09.281122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 076486c8-c419-460a-8e84-30e5137851d1 · inbound

Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620 cites this paper.

Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620 Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Reference 90

Resolution: verified exact; arxiv_id, observed 2026-05-19T02:52:00.049397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 59669975-5c56-4fdd-83f0-ef7a0448c96d · inbound

Persistence of post-Newtonian amplitude structure in binary black hole mergers cites this paper.

Persistence of post-Newtonian amplitude structure in binary black hole mergers Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Reference 54

Resolution: verified exact; arxiv_id, observed 2026-05-18T20:12:50.478176Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation be82c004-05ca-476a-9da0-140a4ab2d5a0 · inbound

First ICCUB Numerical Relativity Waveform Catalog of Eccentric Black Hole Binaries cites this paper.

First ICCUB Numerical Relativity Waveform Catalog of Eccentric Black Hole Binaries Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-15T16:30:11.450740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d16755a5-453c-4e7f-ac78-739d4388547e · inbound

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions cites this paper.

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity

Reference 32

Resolution: metadata mismatch; arxiv_id, observed 2026-05-10T12:10:22.387216Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.