Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2002.11119.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:47:46.643506Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-14T11:47:47.009414Z
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 8c1f52aa-a440-4a5c-a338-27c1b4c3176d · inbound
The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship cites this paper.
The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
Reference 21
- Resolution
- verified exact
- local_arxiv, observed 2026-08-14T11:47:47.014951Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.