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Paper Citation Record · LEDGER

The basic physics of the binary black hole merger GW150914

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1608.01940.

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

pith.paper-citation-record.v1
1608.01940 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T05:10:13.912506Z

measured 1 of 1 external citation measurements

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

105
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b545b9fc-3820-4b44-bea2-e3d82bec9bae · inbound

GW250114: testing Hawking's area law and the Kerr nature of black holes cites this paper.

GW250114: testing Hawking's area law and the Kerr nature of black holes The basic physics of the binary black hole merger GW150914

Reference 15

Resolution
verified exact
arxiv_id, observed 2026-05-13T21:29:44.738451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-13T21:29:44.416458Z digest=sha256:d7034a4d67789abc6c7b64dbe7639def8a9b2e809b08597579af2d23c8d7b941

Observation 227e3714-1835-40c6-aab9-9ea45280bd35 · inbound

Finding Supermassive Black Hole Binary Mergers in Pulsar Timing Array Data cites this paper.

Finding Supermassive Black Hole Binary Mergers in Pulsar Timing Array Data The basic physics of the binary black hole merger GW150914

Reference 75

Resolution
verified exact
local_arxiv, observed 2026-05-18T10:01:13.859619Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-18T09:56:40.692329Z digest=sha256:b58b55e93968ef1952bb83ac8333a84b3cbbcf53ecf34e0ac9bdc0f6e7ff03c0

Observation b6237f7b-52e9-4825-b3b1-d54fa5f30100 · inbound

Polarization Analysis of Ringdown Signals cites this paper.

Polarization Analysis of Ringdown Signals The basic physics of the binary black hole merger GW150914

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-05-19T15:42:38.554097Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-19T15:39:06.963382Z digest=sha256:a7a190bade1d2c2d1b4576906261cf004f917f3e0d58166d108896d34956c3ba

Observation 613ece38-1b90-43c0-930f-c664b0866ec7 · inbound

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions The basic physics of the binary black hole merger GW150914

Reference 128

Resolution
metadata mismatch
local_arxiv, observed 2026-05-22T09:31:22.015565Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f60615756cc9f35669d744d3fe0eff1d425e71435ef1e79bb570d0a211ed6990

Observation b03074f1-4cd4-4e4d-ad82-c012061166f1 · inbound

The SKAO Pulsar Timing Array cites this paper.

The SKAO Pulsar Timing Array The basic physics of the binary black hole merger GW150914

Reference 24

Resolution
unresolved
no resolver link, observed 2026-07-12T05:10:13.912506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T05:10:13.912506Z digest=sha256:a95de63bedee8685444ae669368330f6ec65c32016a14e9d168c9b4875680b35