Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Star formation quenching in simulated group and cluster galaxies: When, how, and why?
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1410.8161.
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 2026-08-06T06:34:29.942622+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 2026-07-02T18:47:16.619058Z
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 3b3e0319-7b51-4e16-80b5-b7678d67db43 · inbound
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation Star formation quenching in simulated group and cluster galaxies: When, how, and why?
Reference 34
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T16:11:01.918975Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation c9c0ce2a-2bb4-46dd-9420-a8bd80df8b12 · inbound
An extreme ram-pressure stripping event in a protocluster at redshift 4.3 cites this paper.
An extreme ram-pressure stripping event in a protocluster at redshift 4.3 Star formation quenching in simulated group and cluster galaxies: When, how, and why?
Reference 12
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T00:10:16.491731Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation ffcca5e0-fec0-40d5-8ce9-4a628a7ebf00 · inbound
Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators cites this paper.
Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators Star formation quenching in simulated group and cluster galaxies: When, how, and why?
Reference 49
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T18:47:16.620370Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.