Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Formation and evolution of protostellar accretion discs. I. Angular-momentum budget, gravitational self-regulation, and numerical convergence
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2101.00131.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T17:19:41.012112Z
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 dd7b373b-44d9-4aca-96dd-b8c3549a51c3 · 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 Formation and evolution of protostellar accretion discs. I. Angular-momentum budget, gravitational self-regulation, and numerical convergence
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:33:53.717649Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e4f456e4-7dd6-48bd-a78b-273f41532a7a · inbound
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.
Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Formation and evolution of protostellar accretion discs. I. Angular-momentum budget, gravitational self-regulation, and numerical convergence
Reference 284
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T17:19:41.012112Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.