Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2406.10757.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T05:54:22.527086Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-18T07:12:26.891121Z
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 55661c86-2fea-4c06-916f-d2f401dbcb08 · inbound
Impact of facility timing and coordination for next-generation gravitational-wave detectors cites this paper.
Impact of facility timing and coordination for next-generation gravitational-wave detectors Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T07:12:26.893454Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation bd7e21f2-6334-4bf4-b1cf-3a65fd48bc22 · inbound
Can machine learning improve the detectability and disentanglement of the gravitational-wave background? cites this paper.
Can machine learning improve the detectability and disentanglement of the gravitational-wave background? Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T00:54:50.170016Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bba5db92-0b06-4bb4-bc29-1863357e7bdc · 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 Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T05:54:22.527086Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.