Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Modeling Galaxies in the Early Universe with Supernova Dust Attenuation
As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2502.14031.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:06:31.589139Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T05:32:42.865600Z
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 299ab944-7e8a-46c9-97d8-c5f03f418797 · inbound
Realistic Multi-temperature Dust: How Well Can We Constrain the Dust Properties of High-redshift Galaxies? cites this paper.
Realistic Multi-temperature Dust: How Well Can We Constrain the Dust Properties of High-redshift Galaxies? Modeling Galaxies in the Early Universe with Supernova Dust Attenuation
Reference 105
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:06:31.589139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 03835b1f-f3ec-4f8f-af3b-73c888c6cf16 · 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 Modeling Galaxies in the Early Universe with Supernova Dust Attenuation
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:38:45.402797Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2c7d2352-2d6c-4d06-a622-1f5c1e36ec19 · inbound
Another view into JWST-discovered X-ray weak AGNs via radiative dusty feedback cites this paper.
Another view into JWST-discovered X-ray weak AGNs via radiative dusty feedback Modeling Galaxies in the Early Universe with Supernova Dust Attenuation
Reference 51
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T05:32:42.874810Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.