Paper Citation Record · LEDGER

What does a binary black hole merger look like?

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1410.7775.

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

pith.paper-citation-record.v1
1410.7775 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T10:10:18.422736Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T08:05:16.230513Z

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 27d086f7-6243-4246-8198-46a9ff2576c1 · inbound

Photon rings and shadows of black holes with non-minimal couplings between curvature and electromagnetic field cites this paper.

Photon rings and shadows of black holes with non-minimal couplings between curvature and electromagnetic field What does a binary black hole merger look like?

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-05-10T08:27:52.096182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 9c35c0a7-dea4-4961-9d25-a879b7e56708 · inbound

Reshaping the inner shadow of a Kerr black hole by a torn accretion disk cites this paper.

Reshaping the inner shadow of a Kerr black hole by a torn accretion disk What does a binary black hole merger look like?

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-05-11T13:51:06.042334Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation e8a317d1-3b2a-4109-80cc-fbac338e6040 · inbound

Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes cites this paper.

Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes What does a binary black hole merger look like?

Reference 130

Resolution: metadata mismatch; local_arxiv, observed 2026-05-15T05:55:04.542380Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation 2053a14e-2a5b-4763-83f4-5db01860b200 · inbound

Polarization-dependent observational signatures of Weyl-coupled photons around a black hole cites this paper.

Polarization-dependent observational signatures of Weyl-coupled photons around a black hole What does a binary black hole merger look like?

Reference 34

Resolution: unresolved; no resolver link, observed 2026-07-14T10:10:18.422736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.