Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
MWC656: A Be+BH or a Be+sdO?
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2208.12315.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.817216Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T12:34:25.264728Z
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 981881f9-4ce5-4aff-a119-07c40c8f015a · inbound
New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling cites this paper.
New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling MWC656: A Be+BH or a Be+sdO?
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:42:29.114759Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5810f9b1-ffe6-4de6-9b19-0cc8cd15622e · inbound
Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814 cites this paper.
Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814 MWC656: A Be+BH or a Be+sdO?
Reference 61
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T12:34:25.267686Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 5630a44b-c64f-4cbc-bb8d-41768cfb8bfa · 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 MWC656: A Be+BH or a Be+sdO?
Reference 264
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.817216Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.