Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1608.07049.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T18:36:54.978114Z
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 6eb96575-3a13-44b2-9826-de534848e45c · inbound
Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? cites this paper.
Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T18:36:54.978114Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 46bdbab9-d15d-4429-a673-ff0a99493383 · inbound
Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars cites this paper.
Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars
Reference 149
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T16:06:33.916254Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.