Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Interstellar dust properties of nearby galaxies
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1711.07434.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T15:21:47.711445Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-14T10:50:24.520610Z
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 9f4c48ad-ec7f-414c-b409-26eba6390195 · inbound
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump cites this paper.
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump The Interstellar dust properties of nearby galaxies
Reference 33
- Resolution
- verified exact
- local_arxiv, observed 2026-07-14T10:50:24.522218Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation bebcb64b-87e0-4660-b3d0-31d1e542d2ca · inbound
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump cites this paper.
Mapping Dust Attenuation at Kiloparsec Scales. III. The 2175\AA\ Bump The Interstellar dust properties of nearby galaxies
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:18:16.889821Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9c155b0e-83ae-4871-921e-ef473c434927 · inbound
Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud cites this paper.
Scylla: Observational Evidence for an Order of Magnitude in Dust Mass Opacity Evolution with ISM Density in the Large Magellanic Cloud The Interstellar dust properties of nearby galaxies
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T15:21:47.711445Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.