Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The spin period - eccentricity relation of double neutron stars: evidence for weak supernova kicks?
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:astro-ph/0507628.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T23:00:46.049637Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-15T23:00:46.336016Z
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 dde08764-b325-450b-91b1-26f9c0cf4fbd · inbound
Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer cites this paper.
Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer The spin period - eccentricity relation of double neutron stars: evidence for weak supernova kicks?
Reference 68
- Resolution
- verified exact
- local_arxiv, observed 2026-08-15T23:00:46.342065Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.