Paper Citation Record · LEDGER

Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2301.07215.

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

pith.paper-citation-record.v1
2301.07215 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:42:50.480887Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T10:41:25.621467Z

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 e21bbeba-1e7f-47a8-8014-5cee99b4444a · inbound

Applications of machine learning in gravitational wave research with current interferometric detectors cites this paper.

Applications of machine learning in gravitational wave research with current interferometric detectors Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

Reference 213

Resolution: unresolved; no resolver link, observed 2026-08-11T11:42:50.480887Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 679c343a-0386-4b16-893b-bee0d8d716b1 · inbound

Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials cites this paper.

Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T22:05:21.878537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d13fbd62-4a8c-4e6f-8345-bdb40c01e09a · 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 Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-03T22:13:48.346507Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8cac23ed-745c-4b3d-b733-1117d5943c89 · inbound

Recoil kicks from binary black hole mergers in GWTC catalogs: implications for retention and hierarchical mergers cites this paper.

Recoil kicks from binary black hole mergers in GWTC catalogs: implications for retention and hierarchical mergers Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-10T22:15:49.414341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 312ec02c-c845-4581-9f7e-62612dba51bc · inbound

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries cites this paper.

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-11T15:01:08.760355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation ce1e3695-b551-462c-bf1a-6d34957aac68 · inbound

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries cites this paper.

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-22T10:41:25.623974Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation b801c02d-daba-4772-b3d3-16da5274f3dd · 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 Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-06T00:42:32.481704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.