Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Connecting a Magnetized Disk to a Convective Low-mass Protostar: A Global Three-dimensional Model of Boundary Layer Accretion
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2503.15350.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T04:54:18.206292Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T08:40:59.943835Z
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 2be6fa1a-1f48-48c0-83c0-a9d5f26b1142 · inbound
Magnetized Accretion onto Neutron Stars: from Photon-trapped to Neutrino-cooled Flows cites this paper.
Magnetized Accretion onto Neutron Stars: from Photon-trapped to Neutrino-cooled Flows Connecting a Magnetized Disk to a Convective Low-mass Protostar: A Global Three-dimensional Model of Boundary Layer Accretion
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T04:54:18.206292Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4fde538a-eb16-45a0-8095-203f1c089891 · inbound
Effect of Magnetic Field on the Accretion Phase of Population III Star Formation cites this paper.
Effect of Magnetic Field on the Accretion Phase of Population III Star Formation Connecting a Magnetized Disk to a Convective Low-mass Protostar: A Global Three-dimensional Model of Boundary Layer Accretion
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T13:44:47.185290Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation acc1a5eb-6723-4249-9e3c-931a6c01abee · inbound
Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation cites this paper.
Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation Connecting a Magnetized Disk to a Convective Low-mass Protostar: A Global Three-dimensional Model of Boundary Layer Accretion
Reference 72
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T08:40:59.946279Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.