Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1805.01484.
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 2026-08-05T10:57:04.762790Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
37
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 1e60c769-7c33-4d94-8dfc-56ac540bd007 · inbound
Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.
Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T10:57:04.762790Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ffddd7ae-1af5-475a-9da3-4aa0534ea217 · inbound
JWST absorption line spectroscopy with SPURS: ISM covering fractions and kinematics in individual galaxies at $z=5-9$ cites this paper.
JWST absorption line spectroscopy with SPURS: ISM covering fractions and kinematics in individual galaxies at $z=5-9$ Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
Reference 94
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T01:51:29.434897Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 7484e362-cbc1-4619-84e1-ebc4ecfbab3f · inbound
JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.
JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
Reference 253
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T18:01:07.906282Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.