Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2005.09759.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T14:01:08.901035Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T14:01:09.602851Z
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 e4737bfb-71db-4ee7-a6e1-d9dd0d41d0af · inbound
Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis cites this paper.
Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T14:01:09.607809Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.