Paper Citation Record · LEDGER

The spectral density of astrophysical stochastic backgrounds

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2411.04028.

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

pith.paper-citation-record.v1
2411.04028 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 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:54:22.572158Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T20:33:58.392994Z

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 3bccc087-f7cb-480b-98d1-8a639e93f730 · inbound

Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background cites this paper.

Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background The spectral density of astrophysical stochastic backgrounds

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-11T04:50:19.412256Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cf3faf3-9dd9-42eb-9cd7-cd5b7c2eb165 · inbound

New test of modified gravity with gravitational wave experiments cites this paper.

New test of modified gravity with gravitational wave experiments The spectral density of astrophysical stochastic backgrounds

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-04T21:14:36.961727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5764bd6e-88ae-45fc-a7b5-cd3055531481 · inbound

Estimating galactic foreground with the population of resolved galactic binaries cites this paper.

Estimating galactic foreground with the population of resolved galactic binaries The spectral density of astrophysical stochastic backgrounds

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-11T13:06:03.141803Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 12e92ed2-1ac6-4daa-8d0c-156bfb486085 · inbound

Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks cites this paper.

Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks The spectral density of astrophysical stochastic backgrounds

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-06-29T20:33:58.394629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 6a901e3a-c3a3-4776-9c48-7888a3f70e9c · inbound

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope The spectral density of astrophysical stochastic backgrounds

Reference 197

Resolution: unresolved; no resolver link, observed 2026-08-01T09:39:05.356034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation caf7ceba-35d6-489f-90c7-a20b6e9a0c93 · 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 The spectral density of astrophysical stochastic backgrounds

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-12T05:54:22.572158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.