Paper Citation Record · LEDGER

Modeling maximum astrophysical gravitational recoil velocities

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1011.0593.

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

pith.paper-citation-record.v1
1011.0593 v1

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measured 0 of 0 reference resolution

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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 2026-08-20T06:33:59.587034+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:50:47.410445Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T09:21:21.030729Z

Reference resolution

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6abb0127-72e9-4a50-8a48-84400183502f · inbound

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

Kicking gravitational wave detectors with recoiling black holes Modeling maximum astrophysical gravitational recoil velocities

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-14T13:50:47.410445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3dae8e2b-de93-44f2-8297-7387edfec9ac · 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 Modeling maximum astrophysical gravitational recoil velocities

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-03T22:13:46.068394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04f8ca25-b5ab-4c1f-83d1-87d323644510 · inbound

Progenitor of the recoiling super-massive black hole RBH-1 identified using HST/JWST imaging cites this paper.

Progenitor of the recoiling super-massive black hole RBH-1 identified using HST/JWST imaging Modeling maximum astrophysical gravitational recoil velocities

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-03T07:54:23.723152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 93bab42e-ffaa-42f8-a802-9674a6bd29e7 · 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 Modeling maximum astrophysical gravitational recoil velocities

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-10T22:15:49.231474Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 8ac7f48b-961b-4bcf-aa0d-d3a28c355bf7 · inbound

GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog cites this paper.

GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog Modeling maximum astrophysical gravitational recoil velocities

Reference 97

Resolution: verified exact; arxiv_id, observed 2026-05-11T00:35:51.411752Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation fde3c8c3-5cf0-4a2f-a950-fe64eaffe625 · inbound

Predicting intermediate-mass black hole formation in star clusters with machine learning cites this paper.

Predicting intermediate-mass black hole formation in star clusters with machine learning Modeling maximum astrophysical gravitational recoil velocities

Reference 130

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:21:21.033421Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation 32250529-ef58-4e95-9540-453ae9051934 · 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 Modeling maximum astrophysical gravitational recoil velocities

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-06T00:42:31.448811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.