Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A new view on the maximum mass of differentially rotating neutron stars
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.02336.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:05:12.192146Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-09T00:07:29.957185Z
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 9fca18db-ad25-419c-86d8-ab1fe0cd2c0a · inbound
Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory cites this paper.
Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory A new view on the maximum mass of differentially rotating neutron stars
Reference 88
- Resolution
- verified exact
- local_arxiv, observed 2026-08-09T00:07:29.960943Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation aed6c372-c3f2-4ccb-b310-459da06ca670 · inbound
Structural quasi-universality in highly magnetized differentially rotating neutron stars cites this paper.
Structural quasi-universality in highly magnetized differentially rotating neutron stars A new view on the maximum mass of differentially rotating neutron stars
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:05:12.192146Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.