Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Possible Formation of Compact Stars in $f(R,T)$ Gravity
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1512.05202.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T12:00:47.307303Z
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 17d5be48-caf9-4fb0-9883-c8f0c184907b · inbound
An innovative black hole solution and thermodynamic properties in higher-order curvature gravity with a scalar field cites this paper.
An innovative black hole solution and thermodynamic properties in higher-order curvature gravity with a scalar field Possible Formation of Compact Stars in $f(R,T)$ Gravity
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T12:00:47.307303Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.