Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A fast and robust recipe for modeling non-ideal MHD effects in star-formation simulations
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2502.06933.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:01:11.361749Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T18:16:16.850658Z
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 3e2bc445-2863-4b79-b3a2-ce2ca526b3dd · inbound
Ambipolar diffusion and the mass-to-flux ratio in a turbulent collapsing cloud cites this paper.
Ambipolar diffusion and the mass-to-flux ratio in a turbulent collapsing cloud A fast and robust recipe for modeling non-ideal MHD effects in star-formation simulations
Reference 4
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-07T14:01:23.513405Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 146ed6bd-d2bf-4b60-b51f-fd5f2f594b1b · inbound
Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs cites this paper.
Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs A fast and robust recipe for modeling non-ideal MHD effects in star-formation simulations
Reference 132
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:34:08.888190Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.