Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2009.04418.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T20:02:43.490063Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-18T07:12:27.014127Z
Reference resolution
0 of 0 outbound references displayed
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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 7b1dd7b0-ebff-4330-a715-8e0b818a4333 · 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 Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:02:43.490063Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a4019c86-7a39-41fd-99d0-40072c4b92dd · inbound
A Fog Over the Cosmological SGWB: Unresolved Massive Black Hole Binaries in the LISA Band cites this paper.
A Fog Over the Cosmological SGWB: Unresolved Massive Black Hole Binaries in the LISA Band Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T18:50:34.550048Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 465320dd-4e63-45b1-b660-31d4400f7b3e · 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 Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
Reference 66
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T07:12:27.016695Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 6f730f8a-488e-40de-8b31-b40188771b36 · inbound
Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors cites this paper.
Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T17:45:19.406341Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c3a627ec-542f-470d-a268-bb6301b27712 · 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? Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T00:54:50.240687Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f6e30f5d-12b8-489c-aec5-65fd40a8a06a · 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 Measuring the primordial gravitational-wave background in the presence of astrophysical foregrounds
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T05:54:22.444536Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.