Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Population of persistent high mass X-ray binaries in the Milky Way
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1302.0728.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T18:24:51.488951Z
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 36c04354-c810-4004-9672-0c8d0a1e8711 · inbound
XMM-Newton follow-up of two eROSITA X-ray binary candidates cites this paper.
XMM-Newton follow-up of two eROSITA X-ray binary candidates Population of persistent high mass X-ray binaries in the Milky Way
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:24:51.488951Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.