Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Bayesian sensitivity of binary pulsars to ultra-light dark matter
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2402.04099.
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 2026-08-16T11:34:36.254170Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-16T10:58:38.068889Z
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 7e243a9d-8767-4a3c-97f3-0c10b3ea2182 · inbound
Discovering $\mu$Hz gravitational waves and ultra-light dark matter with binary resonances cites this paper.
Discovering $\mu$Hz gravitational waves and ultra-light dark matter with binary resonances Bayesian sensitivity of binary pulsars to ultra-light dark matter
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T11:34:36.254170Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d8c9d2e2-2d52-4b97-8718-bd82e8996dba · inbound
Prospects for gravitational wave and ultra-light dark matter detection with binary resonances beyond the secular approximation cites this paper.
Prospects for gravitational wave and ultra-light dark matter detection with binary resonances beyond the secular approximation Bayesian sensitivity of binary pulsars to ultra-light dark matter
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-08-16T10:58:38.075812Z
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.