Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1108.4427.
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 2026-08-07T14:01:09.821081Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T00:45:49.050757Z
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 7a16209b-8641-4339-9dcc-b91a71915450 · inbound
NuSTAR Observations of the Galaxy Cluster Abell 3667 cites this paper.
NuSTAR Observations of the Galaxy Cluster Abell 3667 Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:01:09.821081Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2b42c4f9-fa51-4620-bad7-b857aa44df62 · inbound
The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters cites this paper.
The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \simeq 2$ protoclusters Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters
Reference 106
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T07:56:00.734481Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 28734c14-b451-4206-943a-d9646349a841 · inbound
XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199 cites this paper.
XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199 Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters
Reference 37
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T00:45:49.052046Z
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.