Pith. sign in

Paper Citation Record · LEDGER

Magnetic Field Amplification in Galaxy Clusters and its Simulation

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1810.09783.

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

pith.paper-citation-record.v1
1810.09783 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:22:53.852706Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T18:50:05.600756Z

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 c4029739-6b22-42e3-bc5c-5dac3d13b5e3 · inbound

Active galactic nuclei through the prism of galaxy clusters: bounds on axion-like particles cites this paper.

Active galactic nuclei through the prism of galaxy clusters: bounds on axion-like particles Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-07T11:22:53.852706Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:22:53.852706Z digest=sha256:62216643fe7685af2fcd863092ebd3ab2dc84864f0966436ca427537870af2ea

Observation a0ba70a3-8fc7-4638-8ddc-c0e50b81a0b6 · inbound

Forward cascade of large-scale primordial magnetic fields during structure formation cites this paper.

Forward cascade of large-scale primordial magnetic fields during structure formation Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-06T06:15:10.613668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T06:15:10.613668Z digest=sha256:a946d6f67d4b6866cebe0ec7d189eeed592c62799d95c8ac5c268c1745dcafff

Observation 09e4885f-775f-42bb-9cd5-425ab1706ede · inbound

Constraining AGN accretion physics with black hole mass-luminosity scaling relations cites this paper.

Constraining AGN accretion physics with black hole mass-luminosity scaling relations Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 241

Resolution
verified exact
local_arxiv, observed 2026-06-28T10:12:02.148294Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:cf554e1c1da3c1ebdb029d64deba1caa004e246ce99a5dfb6c1aac072a8c96aa

Observation 2c6c9ebe-18e3-4d41-a143-decf2dd33fe4 · inbound

Symbiotic Magnetogenesis during Radiation Domination cites this paper.

Symbiotic Magnetogenesis during Radiation Domination Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-07-04T18:50:05.601891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-25T22:19:44.658738Z digest=sha256:d4835d88f425f0f09a3d1990ca3771e2f827342c499a0814d23008377f14976c

Observation 30e0622a-671e-4ea2-a098-846875d0d9d3 · inbound

Unraveling the Imprints of Fluctuation-dynamo on the Intracluster Medium with the SKA cites this paper.

Unraveling the Imprints of Fluctuation-dynamo on the Intracluster Medium with the SKA Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 298

Resolution
verified exact
local_arxiv, observed 2026-06-29T04:03:04.978388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8e19fbd81c8acadf88308906f327585556bc5580b81c70c3199808578e984db9

Observation 7d46a48a-a868-46e9-b24e-2cc3273d40d2 · inbound

The Large-Scale Structure of the Universe through the SKA lenses cites this paper.

The Large-Scale Structure of the Universe through the SKA lenses Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 231

Resolution
verified exact
local_arxiv, observed 2026-07-01T04:25:21.731006Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:efdd24144ad3ffae0717de4509168b5ff86072ebbc7f2e8e51be47447d2c3b87

Observation 8793626f-a597-4836-a903-c3ed43340a7f · inbound

Helical radio jets as probes of magnetised cluster environments: Periodic Faraday Rotation Revealed in the Corkscrew Galaxy by POSSUM cites this paper.

Helical radio jets as probes of magnetised cluster environments: Periodic Faraday Rotation Revealed in the Corkscrew Galaxy by POSSUM Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 23

Resolution
unresolved
no resolver link, observed 2026-07-12T07:52:19.107476Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T07:52:19.107476Z digest=sha256:3d55f45527cb89cd2e93ea434848f97c379445a6e69e026f1668644f1e8f7248

Observation b243145a-e6d1-4f6c-8a97-190bd9187614 · inbound

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies cites this paper.

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies Magnetic Field Amplification in Galaxy Clusters and its Simulation

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-06T00:06:26.985848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T00:06:26.985848Z digest=sha256:6684bc8a4d50f2000a7fbb8fd9bfd8ef99bb1c62100fe4c3cb3a63badb2fca86