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 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T04:17:47.054251Z
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 493332a6-96c9-483f-910b-6a9be50311d8 · inbound
Dust emission from the bulk of galaxies at the Epoch of Reionization cites this paper.
Dust emission from the bulk of galaxies at the Epoch of Reionization Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T23:27:14.059546Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ca44aa6c-0169-4d4a-ae0f-6e6c70a4f4fe · inbound
Constraining the link between the 2175{\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI cites this paper.
Constraining the link between the 2175{\AA} dust absorption feature and PAHs in Nearby Star-Forming Galaxies using Swift/UVOT and JWST/MIRI Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T22:18:25.963183Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 608ad5cf-67e0-46f4-9e3f-49f6080ae3c0 · inbound
Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr cites this paper.
Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 143
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T21:08:52.382014Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f450c56d-3d71-4517-8ea8-3c0bd5c0d2b7 · inbound
Deep Swift/UVOT Observations of GOODS-N and the Evolution of the Ultraviolet Luminosity Function at 0.2<z<1.2 cites this paper.
Deep Swift/UVOT Observations of GOODS-N and the Evolution of the Ultraviolet Luminosity Function at 0.2<z<1.2 Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T12:20:41.701402Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5cdcf328-010c-48a2-a2bf-613ece7ab941 · inbound
The Pitfalls of Using Lyman Alpha Damping Wings in High-z Galaxy Spectra to Measure the Intergalactic Neutral Hydrogen Fraction cites this paper.
The Pitfalls of Using Lyman Alpha Damping Wings in High-z Galaxy Spectra to Measure the Intergalactic Neutral Hydrogen Fraction Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T15:34:45.246292Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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 2026-08-15T06:32:42.880941+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.
Observation 5ee76003-a6a4-476d-a6a8-8587b714144a · inbound
Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy cites this paper.
Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T04:17:47.054251Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.