Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Properties of Strong and Weak Propellers from MHD Simulations
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1704.08336.
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 2026-08-12T18:32:10.512463Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
64
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 6f520ce7-2ee4-4fef-b01e-7d94c766d48d · inbound
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 cites this paper.
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 Properties of Strong and Weak Propellers from MHD Simulations
Reference 219
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:58:09.313741Z
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 930d09f3-edfd-4f3a-9385-ef28f3aff48a · 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? Properties of Strong and Weak Propellers from MHD Simulations
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T18:32:10.512463Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.