Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Characterizing the nanohertz gravitational wave background using a $t$-process power spectral density
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2408.10139.
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 2026-08-04T22:54:55.912592Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T09:56:10.473001Z
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 d2e798d4-7a30-4220-97af-4bc886da9b57 · inbound
Mapping the Gravitational-wave Background Across the Spectrum with a Next-Generation Anisotropic Per-frequency Optimal Statistic cites this paper.
Mapping the Gravitational-wave Background Across the Spectrum with a Next-Generation Anisotropic Per-frequency Optimal Statistic Characterizing the nanohertz gravitational wave background using a $t$-process power spectral density
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T22:54:55.912592Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d763116-ada4-4d45-8b6a-eed180afeb9e · inbound
A Joint Optimal Search for Gravitational Waves from Resolved and Unresolved Supermassive Binary Black Holes with Pulsar Timing Arrays cites this paper.
A Joint Optimal Search for Gravitational Waves from Resolved and Unresolved Supermassive Binary Black Holes with Pulsar Timing Arrays Characterizing the nanohertz gravitational wave background using a $t$-process power spectral density
Reference 32
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T23:09:01.214159Z
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 93f49ce3-75d2-48ae-9e07-74bc911bc7e2 · inbound
Population statistics of nanohertz gravitational wave sources cites this paper.
Population statistics of nanohertz gravitational wave sources Characterizing the nanohertz gravitational wave background using a $t$-process power spectral density
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T09:56:10.474828Z
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.