Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2412.03662.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T05:22:21.386491Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T06:16:20.379382Z
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 c1e2e3ad-996c-4ffd-b701-cc754afe2f91 · inbound
Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos cites this paper.
Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos The Growth of Galaxy Stellar Haloes Over $0.2 \leq z \leq 1.1$
Reference 82
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-05T05:22:21.924162Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.