Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Revisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2104.13148.
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 2026-08-07T20:40:57.154700Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
44
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 9816f195-1ec0-423c-a564-561ffcb98adf · inbound
SAS in ESA Datalabs: A New Platform for XMM-Newton Analysis cites this paper.
SAS in ESA Datalabs: A New Platform for XMM-Newton Analysis Revisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge
Reference 2021
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:21:15.813680Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0eb3afe2-0dec-400a-8095-6fb70e0d1708 · inbound
Blind Line Search System: BLiSS cites this paper.
Blind Line Search System: BLiSS Revisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge
Reference 19
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T18:17:33.604439Z
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 6c6d4e47-3760-454c-93df-4ad968ac7dde · 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 Revisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.154700Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.