Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2402.05996.
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 2026-08-05T14:38:44.621981Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation cac59902-31c6-45dc-98df-400c58a22861 · inbound
Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions cites this paper.
Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:38:44.621981Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 263d3a85-10bf-4606-a4ec-65fb49c60959 · inbound
Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations cites this paper.
Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-06-27T15:51:01.553494Z
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 c86f5916-3d69-4be9-9b14-f0a17cff53a8 · inbound
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.
The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T00:50:15.126886Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.