Paper Citation Record · LEDGER

Time-dependence of the astrophysical stochastic gravitational wave background

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1912.07657.

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

pith.paper-citation-record.v1
1912.07657 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T18:12:53.951102Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T01:55:55.821309Z

Reference resolution

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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 6818e984-b263-43d7-90c7-35fffdff58be · inbound

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes cites this paper.

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes Time-dependence of the astrophysical stochastic gravitational wave background

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-12T18:12:01.392768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 484a1bc7-5980-4e87-b499-89da766f5b15 · inbound

Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order cites this paper.

Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order Time-dependence of the astrophysical stochastic gravitational wave background

Reference 189

Resolution: verified exact; arxiv_id, observed 2026-05-22T01:55:55.823042Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 4cd251c0-fa68-4ba8-a02b-41cfc623060a · inbound

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys cites this paper.

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys Time-dependence of the astrophysical stochastic gravitational wave background

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T04:21:33.067844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d59f5c56-5191-4eff-8ff0-b67035d99dc1 · inbound

Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge cites this paper.

Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge Time-dependence of the astrophysical stochastic gravitational wave background

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T00:25:51.887575Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f9fca9b-84a3-4c16-8c0e-a2488bba821a · inbound

A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background cites this paper.

A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background Time-dependence of the astrophysical stochastic gravitational wave background

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-15T18:12:53.951102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4573d1f-92f1-48ba-9a2f-6b813de9b753 · inbound

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background cites this paper.

All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background Time-dependence of the astrophysical stochastic gravitational wave background

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.459467Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.