Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining the neutron star equation of state using Pulse Profile Modeling
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1904.07012.
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 2026-08-08T12:40:54.737873Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-24T22:25:01.609084Z
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 1496aa53-495f-4e1c-af27-31e2258add41 · inbound
Compact star properties from an extended linear sigma model cites this paper.
Compact star properties from an extended linear sigma model Constraining the neutron star equation of state using Pulse Profile Modeling
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T22:25:01.612104Z
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.
Observation 12341ece-e14e-4819-9b01-91c0d736a254 · inbound
Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate cites this paper.
Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate Constraining the neutron star equation of state using Pulse Profile Modeling
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T12:40:54.737873Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.