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Paper Citation Record · LEDGER

Properties of clumps and filaments around galaxy clusters

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2102.01096.

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

pith.paper-citation-record.v1
2102.01096 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.530483Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

27
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3597f6be-aa2e-4efd-aeae-8ffaccee80cc · inbound

A Detailed View of the Large-Scale Sloshing Cold Front in RXJ2014.8-2430 cites this paper.

A Detailed View of the Large-Scale Sloshing Cold Front in RXJ2014.8-2430 Properties of clumps and filaments around galaxy clusters

Reference 110

Resolution
verified exact
arxiv_id, observed 2026-05-11T15:16:07.546400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-05-09T20:25:47.917486Z digest=sha256:d8f054dd54668b02992770be0f500fb22e556f34db79ee5fb0a6418e38cfbd0c

Observation c99cd6fc-c83c-4a5a-a177-93204c63930b · inbound

The Treble Clef radio phoenix and its old nonthermal filaments cites this paper.

The Treble Clef radio phoenix and its old nonthermal filaments Properties of clumps and filaments around galaxy clusters

Reference 139

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T23:57:46.743657Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:12faa2a563f6394015477fd042ab4a414452af0aa37bd88f4f87b877a15081ef

Observation eec84b0a-c753-40a0-b731-9136e3feeabf · inbound

The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field cites this paper.

The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field Properties of clumps and filaments around galaxy clusters

Reference 139

Resolution
unresolved
no resolver link, observed 2026-08-02T02:52:01.173500Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:52:01.173500Z digest=sha256:77154173f6a38f31d840506c42ea9a4051fafd73347acbc58c3ec747db006fe9

Observation 0bdecf8b-26e1-4696-be18-cbd77552d382 · inbound

Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations cites this paper.

Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations Properties of clumps and filaments around galaxy clusters

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-10T04:15:20.530483Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:15:20.530483Z digest=sha256:6f20bbd499d069c23564e9204fd764bac75c6a256fe41f08733c1cdf96147015