Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The PAH emission characteristics of the reflection nebula NGC2023
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1701.06585.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T21:40:11.483704Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-20T08:43:09.711200Z
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 8a0cd60d-d282-45fb-8e6d-eb34290be510 · inbound
Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference" cites this paper.
Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference" The PAH emission characteristics of the reflection nebula NGC2023
Reference 145
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:43:09.713023Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 38faaa42-ec76-41b2-9295-0fcd98a167b9 · inbound
Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band cites this paper.
Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band The PAH emission characteristics of the reflection nebula NGC2023
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T21:40:11.483704Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.