Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Learning the Universe: physically-motivated priors for dust attenuation curves
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2502.13240.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T11:34:45.494235Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T14:38:50.873653Z
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 2360d8f1-d02e-472c-ac65-f493248bb775 · inbound
Big, Dusty Galaxies in Blue Jay: Insights into the Relationship Between Morphology and Dust Attenuation at Cosmic Noon cites this paper.
Big, Dusty Galaxies in Blue Jay: Insights into the Relationship Between Morphology and Dust Attenuation at Cosmic Noon Learning the Universe: physically-motivated priors for dust attenuation curves
Reference 113
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T11:34:45.494235Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e60e9277-4bb1-4c3e-9490-a4fffdc8cb55 · 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 Learning the Universe: physically-motivated priors for dust attenuation curves
Reference 113
- Resolution
- verified exact
- local_arxiv, observed 2026-08-05T14:38:50.961756Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation db85980d-de79-4dab-8b76-64364b53cf06 · inbound
Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping cites this paper.
Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping Learning the Universe: physically-motivated priors for dust attenuation curves
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T12:40:12.991313Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.