Paper Citation Record · LEDGER

Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2010.02135.

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

pith.paper-citation-record.v1
2010.02135 v2

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 2026-08-23T06:30:58.430688+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:59:38.783958Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T14:11:05.022911Z

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 a205e7e8-2250-49df-a452-1e668171c229 · inbound

Inferring the cosmological constant in early Universe only by gravitational waves cites this paper.

Inferring the cosmological constant in early Universe only by gravitational waves Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T17:04:42.622668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d903bfdc-38ca-449f-8e8e-a05795c1d9d5 · inbound

Exploring Ultralight Dark Matter Self-Coupling via the Gravitational Wave Background cites this paper.

Exploring Ultralight Dark Matter Self-Coupling via the Gravitational Wave Background Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-16T05:59:38.783958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc90d12a-079f-4d28-86f9-d9d27c1fe5e9 · inbound

Resonant Loop Interferometers for High-Frequency Gravitational Waves cites this paper.

Resonant Loop Interferometers for High-Frequency Gravitational Waves Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-04T09:47:47.035234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 440e33ad-1c7d-42bc-bdda-f777721d963a · inbound

Gravity Echoes from Supermassive Black Hole Binaries cites this paper.

Gravity Echoes from Supermassive Black Hole Binaries Sensitivity of present and future detectors across the black-hole binary gravitational wave spectrum

Reference 40

Resolution: verified exact; arxiv_id, observed 2026-05-11T14:11:05.024973Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.