Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1509.07870.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:07:32.102180Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 bf476c1d-5b1b-497d-be9f-835af84dfc8a · inbound
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
Reference 92
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:42:37.987978Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 54c1faf2-285d-436f-a263-2e8da55c88a1 · inbound
Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation cites this paper.
Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation The galaxy luminosity function in groups and clusters: the faint-end upturn and the connection to the field luminosity function
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:07:32.102180Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.