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Paper Citation Record · LEDGER

The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1505.06962.

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

pith.paper-citation-record.v1
1505.06962 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 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T22:32:29.034471Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-17T21:43:30.378795Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 54b22354-5875-4616-8520-c26a6fb86dd3 · inbound

Science with the Einstein Telescope: a comparison of different designs cites this paper.

Science with the Einstein Telescope: a comparison of different designs The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region

Reference 126

Resolution
verified exact
local_arxiv, observed 2026-05-17T21:43:30.380681Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-17T21:43:29.760310Z digest=sha256:b44eb8a82ed6f136ed93ad4b8418c1a3d8543793f05aa5d93236d33d795eb4fd

Observation 164a5ac3-b665-485b-98d4-caea937a9c79 · inbound

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories cites this paper.

Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-07T22:32:29.034471Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T22:32:29.034471Z digest=sha256:4e474bde4c516430281e90a6601e47345c69cfd71344e6f88a806cfbd3aad073