Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Recurrent low-level luminosity behaviour after a giant outburst in the Be/X-ray transient 4U 0115+63
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1907.04724.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T13:59:24.153222Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T13:59:24.239467Z
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 15774b6e-f9ef-4930-bd27-4596aff4d49a · inbound
The frequency of Kozai-Lidov disc oscillation driven giant outbursts in Be/X-ray binaries cites this paper.
The frequency of Kozai-Lidov disc oscillation driven giant outbursts in Be/X-ray binaries Recurrent low-level luminosity behaviour after a giant outburst in the Be/X-ray transient 4U 0115+63
Reference 76
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-14T13:59:24.247079Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation efb603f6-eecc-4c6e-8f42-54a8f1d4f975 · 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 Recurrent low-level luminosity behaviour after a giant outburst in the Be/X-ray transient 4U 0115+63
Reference 249
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.760612Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8fbc9cd5-ff04-4258-a603-dae7cf4c091d · inbound
Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? cites this paper.
Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? Recurrent low-level luminosity behaviour after a giant outburst in the Be/X-ray transient 4U 0115+63
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T18:32:10.472948Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.