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Paper Citation Record · LEDGER

An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2004.09288.

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

pith.paper-citation-record.v1
2004.09288 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T17:33:38.527281Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T05:23:57.234467Z

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 dc4ffdec-6714-41a7-a6f7-d93fe3896f9d · inbound

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run cites this paper.

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary

Reference 65

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:30:26.349004Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T09:30:24.998354Z digest=sha256:85029b4d3ca52e63fb8e35dc94d0e2aa42e04e16fcf6673a88323b05f0cd9de6

Observation 97882d3a-262b-4cf4-a3e4-d2e312072a41 · inbound

Waveform Modelling for the Laser Interferometer Space Antenna cites this paper.

Waveform Modelling for the Laser Interferometer Space Antenna An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary

Reference 211

Resolution
verified exact
arxiv_id, observed 2026-05-24T05:23:57.237231Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-24T05:21:16.199631Z digest=sha256:e4d0c1ce5e20d7aac3cad58802f3a93b8b0f0cad67f6f7e38d72c709d0c6ef9e

Observation 8ff85f19-cb90-48d4-b81c-f2225be0bdff · inbound

Secondary spins of extreme mass ratio inspirals: A probe to the formation channels cites this paper.

Secondary spins of extreme mass ratio inspirals: A probe to the formation channels An alternative interpretation of GW190412 as a binary black hole merger with a rapidly spinning secondary

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-09T17:33:38.527281Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T17:33:38.527281Z digest=sha256:390da13a61a9543f29906850a4dcf4ec47e7bfe909b17b6b061f8229979ce4a7