Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
JADES: Physical properties of Ly$\alpha$ and non-Ly$\alpha$ emitters at z ~ 4.8-9.6
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2406.11997.
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 2026-08-07T23:58:54.297674Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
6
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation cb428d52-ea02-43be-b710-2ca27e011d9c · inbound
The AURORA Survey: The Evolution of Multi-phase Electron Densities at High Redshift cites this paper.
The AURORA Survey: The Evolution of Multi-phase Electron Densities at High Redshift JADES: Physical properties of Ly$\alpha$ and non-Ly$\alpha$ emitters at z ~ 4.8-9.6
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T23:58:54.297674Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1f5904f-b2dc-499e-a92a-87a1eb652411 · inbound
pySTARBURST99: The Next Generation of STARBURST99 cites this paper.
pySTARBURST99: The Next Generation of STARBURST99 JADES: Physical properties of Ly$\alpha$ and non-Ly$\alpha$ emitters at z ~ 4.8-9.6
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T12:35:45.909192Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 12e8db93-64e3-4e9e-b2f9-50f5eae5a5a6 · inbound
Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities cites this paper.
Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities JADES: Physical properties of Ly$\alpha$ and non-Ly$\alpha$ emitters at z ~ 4.8-9.6
Reference 109
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T22:29:58.855518Z
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.