Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the stability and maximum mass of differentially rotating relativistic stars
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1709.06058.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T00:21:42.924335Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T21:58:59.630644Z
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 645953d0-397a-4811-b124-82913428ab3a · 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 On the stability and maximum mass of differentially rotating relativistic stars
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T00:07:29.627697Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1a74b729-5214-4315-9b9e-0b5e822933eb · inbound
Hybrid Stars with Post-Merger Rotation Profiles cites this paper.
Hybrid Stars with Post-Merger Rotation Profiles On the stability and maximum mass of differentially rotating relativistic stars
Reference 21
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T21:58:59.631854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 74a6e8f6-7c7f-44fa-a72f-cc8ed26a8e21 · inbound
Transport properties in binary neutron star mergers: Effect of magnetic field cites this paper.
Transport properties in binary neutron star mergers: Effect of magnetic field On the stability and maximum mass of differentially rotating relativistic stars
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:42.924335Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.