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Paper Citation Record · LEDGER

Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters

As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1108.4427.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1108.4427 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-07-23T06:31:01.910684+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T07:56:00.734481Z

measured 0 of 1 external citation measurements

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 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.

source=arxiv_source observed=2026-07-12T07:56:00.734481Z digest=sha256:3fbd2feda38aaba49cc25f06a7d7db6aa239ea925cad4e14bc44d34c99515b6d

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 2026-07-23T06:31:01.910684+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:131a4d43e52755b41cc33d2a83c619e7362791470ae575ba2c8a2a9db66f6681