Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Maximal Mass Neutron Star as a Key to Superdense Matter Physics
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.16847.
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 2026-08-10T14:01:08.634642Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T04:06:35.460176Z
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 086f5b44-344d-4ac8-8089-2228e65e1711 · 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 Maximal Mass Neutron Star as a Key to Superdense Matter Physics
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T14:01:08.634642Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 062e0b6f-8902-4dc6-9130-19c096d1ae80 · inbound
Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements cites this paper.
Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements Maximal Mass Neutron Star as a Key to Superdense Matter Physics
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T04:06:35.461473Z
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.