Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1506.03600.
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 2026-08-11T05:41:09.792126Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-14T12:30:27.855430Z
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 56871f94-947a-4c19-b258-75b1ed6388ad · 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 On the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources
Reference 294
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T05:41:09.792126Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bd126bbe-b43d-465c-b6b5-c9f4cfc0c2d3 · inbound
Physics of Strong Magnetism with eXTP cites this paper.
Physics of Strong Magnetism with eXTP On the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources
Reference 263
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:19:09.811458Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4935676d-1bac-46c9-bf82-2c1ddabe1aa7 · inbound
Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion cites this paper.
Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion On the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources
Reference 22
- Resolution
- verified exact
- local_arxiv, observed 2026-07-14T12:30:27.857155Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.