Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The time evolution of $M_{\mathrm{d}}/\dot M$ in protoplanetary discs as a way to disentangle between viscosity and MHD winds
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2309.04496.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T01:36:10.749671Z
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 92f13f6c-01d2-47cc-bf51-d880cae8b9a4 · inbound
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments The time evolution of $M_{\mathrm{d}}/\dot M$ in protoplanetary discs as a way to disentangle between viscosity and MHD winds
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-07-30T14:23:16.682703Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fff0b0d8-9e1d-4b63-8690-e97929d62332 · inbound
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.
Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments The time evolution of $M_{\mathrm{d}}/\dot M$ in protoplanetary discs as a way to disentangle between viscosity and MHD winds
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T01:36:10.749671Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.