Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1901.11276.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:37:52.402051Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T14:37:57.563027Z
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 6df8ff57-5919-46e2-93e7-c0cc2d448a8e · inbound
Cosmological feedback from a halo assembly perspective cites this paper.
Cosmological feedback from a halo assembly perspective LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
Reference 54
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T14:37:57.642100Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation dc39009d-6fbd-4269-8544-10dd8bdd8905 · inbound
Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations cites this paper.
Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T06:10:12.293568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.