Paper Citation Record · LEDGER

How black holes get their kicks: Gravitational radiation recoil revisited

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0402056.

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

pith.paper-citation-record.v1
astro-ph/0402056 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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 2026-08-14T06:32:32.682623+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:32:50.649118Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T22:15:49.416507Z

Reference resolution

0 of 0 outbound references displayed

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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 8e3ca6a4-5fc5-476d-833e-984680ad46cb · inbound

Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity cites this paper.

Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity How black holes get their kicks: Gravitational radiation recoil revisited

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-06T21:32:50.649118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 385b050e-e904-471d-9f03-670445141924 · 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 How black holes get their kicks: Gravitational radiation recoil revisited

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-03T22:13:48.993591Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f2c04368-e0b5-4e52-926f-4e9f37ad8a66 · 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 How black holes get their kicks: Gravitational radiation recoil revisited

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-07-04T16:42:57.407956Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 00963b3c-5560-45ee-a310-a1a004742ff4 · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins How black holes get their kicks: Gravitational radiation recoil revisited

Reference 22

Resolution: unresolved; no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f27bb9d-8150-4c2a-a298-c9573c2f9739 · inbound

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations cites this paper.

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations How black holes get their kicks: Gravitational radiation recoil revisited

Reference 80

Resolution: unresolved; no resolver link, observed 2026-07-31T01:54:12.350231Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7f09885-17f7-4f0e-976f-a87b049b3dd2 · 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 How black holes get their kicks: Gravitational radiation recoil revisited

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T00:42:34.914366Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.