Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
High-Mass X-ray Binaries in the Milky Way: A closer look with INTEGRAL
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1505.03651.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:41:13.728192Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 0b4436db-3de8-45f1-ae78-14be9cab3fc0 · inbound
X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries cites this paper.
X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries High-Mass X-ray Binaries in the Milky Way: A closer look with INTEGRAL
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T05:41:08.801655Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 59da6e35-275a-4ec2-a353-94b2fc908c98 · 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 High-Mass X-ray Binaries in the Milky Way: A closer look with INTEGRAL
Reference 158
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.413332Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8ffcb745-4213-498c-a6b7-f1c60b9e117a · 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 High-Mass X-ray Binaries in the Milky Way: A closer look with INTEGRAL
Reference 158
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:41:13.728192Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.