Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Disk kinematics at high redshift: DysmalPy's extension to 3D modeling and comparison with different approaches
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2411.07312.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T20:15:33.746098Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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- 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 605fd5f0-821a-4596-af18-9a76ca1119a7 · inbound
Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics cites this paper.
Assessing the dark matter content of two quasar host galaxies at z~6 through gas kinematics Disk kinematics at high redshift: DysmalPy's extension to 3D modeling and comparison with different approaches
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T20:15:33.746098Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed3e09dd-d0c0-4881-98ed-55b8ec3cf860 · inbound
Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension cites this paper.
Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension Disk kinematics at high redshift: DysmalPy's extension to 3D modeling and comparison with different approaches
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T15:29:48.756185Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.