Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Probing mass-radius relation of protoneutron stars from gravitational-wave asteroseismology
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1708.03738.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T04:16:46.643709Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T04:16:48.919843Z
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 072fcb1a-2b40-4b14-8feb-944da4837e88 · inbound
On the nature of oscillating modes of proto-neutron stars cites this paper.
On the nature of oscillating modes of proto-neutron stars Probing mass-radius relation of protoneutron stars from gravitational-wave asteroseismology
Reference 48
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T04:16:48.931463Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.