Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2006.16116.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T20:02:43.498922Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T00:25:56.369116Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 605a9ac0-5ac7-48ea-8f3f-056bc0879cae · 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 Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T00:25:56.419606Z
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.
Observation 53bb82e9-ad6a-4adc-a2ab-f7cf0b9a0441 · inbound
The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise cites this paper.
The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Searching for cosmological gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:02:43.498922Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0d5e9bd0-4eb2-48e0-8be5-c5ae533d7afa · 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 gravitational-wave backgrounds with third-generation detectors in the presence of an astrophysical foreground
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T00:54:49.973875Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.