Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A New Two-Fluid Radiation-Hydrodynamical Model for X-ray Pulsar Accretion Columns
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1612.02411.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T18:32:10.740727Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-01T01:55:14.977483Z
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 63083ce5-1554-47d3-96a8-bb67818bad8c · inbound
A New Relativistic Model for Spectral Formation in Accretion-Powered X-ray Pulsars: Pulse Profiles and Phase-Averaged Spectra cites this paper.
A New Relativistic Model for Spectral Formation in Accretion-Powered X-ray Pulsars: Pulse Profiles and Phase-Averaged Spectra A New Two-Fluid Radiation-Hydrodynamical Model for X-ray Pulsar Accretion Columns
Reference 155
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T01:55:14.978715Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation d2a85199-ab61-4a3e-83b9-4373520ed9f9 · inbound
Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? cites this paper.
Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? A New Two-Fluid Radiation-Hydrodynamical Model for X-ray Pulsar Accretion Columns
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T18:32:10.740727Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.