Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
X-ray emission from interacting massive binaries: a review of 15 years of progress
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1509.06480.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T13:33:06.674749Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-08T13:33:08.327827Z
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 6405e83c-8e13-43e7-a954-ca1aac8071d7 · inbound
A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179 cites this paper.
A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179 X-ray emission from interacting massive binaries: a review of 15 years of progress
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T17:48:13.854594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a9bfe3d0-ed64-417a-b086-66c8c64d6e76 · inbound
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars X-ray emission from interacting massive binaries: a review of 15 years of progress
Reference 135
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-08T13:33:08.331359Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.