Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A unified accretion-ejection paradigm for black hole X-ray binaries. VI. Radiative efficiency and radio-X-ray correlation during four outbursts from GX339-4
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2109.13592.
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 2026-08-05T10:32:52.528417Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T10:32:54.841384Z
Reference resolution
0 of 0 outbound references displayed
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- 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 a5f44e3d-3226-4899-acbb-a589179f8a3f · inbound
Single spin asymmetry $A _ { U L } ^ { \sin ( 3 \phi _ { h } - \phi_{ R } ) }$ in dihadron production in SIDIS cites this paper.
Single spin asymmetry $A _ { U L } ^ { \sin ( 3 \phi _ { h } - \phi_{ R } ) }$ in dihadron production in SIDIS A unified accretion-ejection paradigm for black hole X-ray binaries. VI. Radiative efficiency and radio-X-ray correlation during four outbursts from GX339-4
Reference 41
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T10:32:54.888084Z
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 30b96789-3a76-46fc-a6a9-318a15cada59 · inbound
How massive and clumpy must a quasar wind be to create emission line blueshifts? cites this paper.
How massive and clumpy must a quasar wind be to create emission line blueshifts? A unified accretion-ejection paradigm for black hole X-ray binaries. VI. Radiative efficiency and radio-X-ray correlation during four outbursts from GX339-4
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T03:00:27.604927Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.