Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
What is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1402.1168.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-27T18:01:08.035925Z
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 923b0e98-5228-48f2-9647-03ee45f4e096 · inbound
JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.
JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe What is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters
Reference 208
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T18:01:08.037472Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 6b5ba94e-3b24-4bbb-90cb-c6ea75ad80c3 · inbound
Lyman-alpha haloes in the aftermath of reionisation cites this paper.
Lyman-alpha haloes in the aftermath of reionisation What is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters
Reference 81
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T09:01:37.245115Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.