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Paper Citation Record · LEDGER

Prospects for estimating parameters from gravitational waves of superspinar binaries

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2104.12968.

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

pith.paper-citation-record.v1
2104.12968 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:58:53.750643Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T08:16:00.523269Z

Reference resolution

0 of 0 outbound references displayed

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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 c2f0d09a-0cc0-40ca-ad05-b34de70ade23 · inbound

Testing the nature of compact objects in the lower mass gap using gravitational wave observations cites this paper.

Testing the nature of compact objects in the lower mass gap using gravitational wave observations Prospects for estimating parameters from gravitational waves of superspinar binaries

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-15T15:58:53.750643Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T15:58:53.750643Z digest=sha256:b4503a8384b1ec9a806fb139549a5f87f61ff6563022f913e13d1fedc59bb8a7

Observation 4bf22e57-3b37-490e-9f4a-0cae903afe8d · inbound

Testing the Kerr hypothesis beyond the quadrupole with GW241011 cites this paper.

Testing the Kerr hypothesis beyond the quadrupole with GW241011 Prospects for estimating parameters from gravitational waves of superspinar binaries

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-05-11T08:16:00.526121Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-10T16:45:03.010161Z digest=sha256:d6f5979f4115e55b1fffced334f99241c4bd7381e7ff63d40fc00dbb1a888f0c