Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Hot third family of compact stars and the possibility of core-collapse supernova explosions
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1511.06551.
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 2026-08-12T14:48:39.981339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T14:48:40.040488Z
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 1d723bca-f28c-44e5-b9e3-f8ec9179290a · inbound
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state cites this paper.
Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state Hot third family of compact stars and the possibility of core-collapse supernova explosions
Reference 78
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:48:40.046932Z
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 3b078e86-f68c-4333-a7ab-0b14a3f9027a · inbound
The petit four of color-superconducting phases in proto-neutron star evolution cites this paper.
The petit four of color-superconducting phases in proto-neutron star evolution Hot third family of compact stars and the possibility of core-collapse supernova explosions
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T04:54:21.953406Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.