Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A catalogue and statistical analysis for magnetic stars
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2307.12315.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.516901Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T20:04:36.552680Z
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 7b5d1f24-8a22-41c5-9525-b471c9b8f406 · inbound
Pre-main Sequence B Stars Surrounding the Orion Nebula cites this paper.
Pre-main Sequence B Stars Surrounding the Orion Nebula A catalogue and statistical analysis for magnetic stars
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:32:50.528770Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5f3ca5b0-52a1-4c2b-abd7-8b15dc284e98 · inbound
The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.
The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry A catalogue and statistical analysis for magnetic stars
Reference 153
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T20:04:36.627242Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 6848b95c-b5ca-4020-9d1f-c7b2274327cf · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry A catalogue and statistical analysis for magnetic stars
Reference 185
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.516901Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.