Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining the properties of the proposed supermassive black hole system in 3c66b: Limits from pulsar timing
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:astro-ph/0310276.
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 2026-08-01T00:47:55.311505Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 6037cc6b-fa77-4ac5-9241-3bdf8aba9111 · inbound
QuickGWecc: Fast Bayesian pipeline for searching eccentric binaries in pulsar timing array data cites this paper.
QuickGWecc: Fast Bayesian pipeline for searching eccentric binaries in pulsar timing array data Constraining the properties of the proposed supermassive black hole system in 3c66b: Limits from pulsar timing
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:47:55.311505Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.