Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dependence of galaxy clustering on UV-luminosity and stellar mass at $z \sim 4 - 7$
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1809.10161.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T14:10:56.781404Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-01T04:05:20.445051Z
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 9227b849-58ab-4648-bac7-d4d2350428bc · inbound
COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? cites this paper.
COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? Dependence of galaxy clustering on UV-luminosity and stellar mass at $z \sim 4 - 7$
Reference 123
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T04:05:20.446261Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 09831611-be4f-4d46-8903-68bd3ba178e7 · inbound
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Dependence of galaxy clustering on UV-luminosity and stellar mass at $z \sim 4 - 7$
Reference 176
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:56.781404Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.