Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Colliding black holes: how far can the close approximation go?
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:gr-qc/9609022.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
125
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation a52ea9bb-ff8d-49b2-a600-7e6cd934b4af · inbound
Quasinormal modes of black holes and black branes cites this paper.
Quasinormal modes of black holes and black branes Colliding black holes: how far can the close approximation go?
Reference 87
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:59:53.120236Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 9b996e7a-17e7-4bef-a5a9-b13c8f682de2 · inbound
GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$ cites this paper.
GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$ Colliding black holes: how far can the close approximation go?
Reference 65
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-16T03:16:33.933514Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation ad6eb45b-4739-4d76-9cfa-c71495750904 · inbound
Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms cites this paper.
Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms Colliding black holes: how far can the close approximation go?
Reference 173
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T10:19:21.011788Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 46330f19-9d83-4cc1-a207-f6ccc3eeba17 · inbound
Black Hole Ringdown Nonlinearities in the Large-D Limit cites this paper.
Black Hole Ringdown Nonlinearities in the Large-D Limit Colliding black holes: how far can the close approximation go?
Reference 13
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T12:09:48.478758Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation f90683ac-86a1-491f-a444-24226eb0054e · inbound
Foundations of Direct Waves in Schwarzschild Ringdown cites this paper.
Foundations of Direct Waves in Schwarzschild Ringdown Colliding black holes: how far can the close approximation go?
Reference 71
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T23:37:41.424114Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 2803d540-c824-414b-ab2b-5591cdfe6829 · inbound
Quasi-Normal Modes of Stars and Black Holes cites this paper.
Quasi-Normal Modes of Stars and Black Holes Colliding black holes: how far can the close approximation go?
Reference 101
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T02:26:20.266171Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.