Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2004.01205.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T18:26:36.462946Z
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 0d23f36d-fb3b-4432-abf2-a2055c803f8f · inbound
High Power Accretion in Massive Binary Systems and the Impact of Metallicity cites this paper.
High Power Accretion in Massive Binary Systems and the Impact of Metallicity The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T18:26:36.462946Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 38d1ba54-96ec-4541-b007-0404093a5973 · inbound
Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook cites this paper.
Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T05:12:17.050532Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.