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Paper Citation Record · LEDGER

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM

As of 23 August 2026, this Paper Citation Record lists 81 of 81 outbound references and 0 inbound Pith citation observations for arXiv:2607.06346.

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

pith.paper-citation-record.v1
2607.06346 v1

Coverage vector

measured 81 of 81 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 81 of 81 standing notices

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

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

81 of 81 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation b983dd48-6c4c-4279-9644-da8f9697fa00 · outbound

This paper cites Residual Gas Motions in the Intracluster Medium and Bias in Hydrostatic Measurements of Mass Profiles of Clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Residual Gas Motions in the Intracluster Medium and Bias in Hydrostatic Measurements of Mass Profiles of Clusters

Reference 1

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Observation fce89def-cba3-4bd9-87f3-36c2f240da6a · outbound

This paper cites Turbulence and Vorticity in Galaxy Clusters Generated by Structure Formation.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Turbulence and Vorticity in Galaxy Clusters Generated by Structure Formation

Reference 2

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local_arxiv, observed 2026-07-08T09:14:46.843736Z

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Observation 409cfc8f-749c-4914-96f1-1b4002353fc8 · outbound

This paper cites The Matryoshka Run (II): Time Dependent Turbulence Statistics, Stochastic Particle Acceleration and Microphysics Impact in a Massive Galaxy Cluster.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The Matryoshka Run (II): Time Dependent Turbulence Statistics, Stochastic Particle Acceleration and Microphysics Impact in a Massive Galaxy Cluster

Reference 3

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local_arxiv, observed 2026-07-08T09:14:46.797256Z

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Observation c391ae87-3c59-4b86-8976-20f3d8e6eb61 · outbound

This paper cites Characteristic Lengths of Magnetic Field in Magnetohydrodynamic Turbulence.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Characteristic Lengths of Magnetic Field in Magnetohydrodynamic Turbulence

Reference 4

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local_arxiv, observed 2026-07-08T09:14:46.744539Z

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Observation fca966fc-245b-4262-a9f0-ff1c6708ca4e · outbound

This paper cites A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417

Reference 5

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arxiv_id, observed 2026-07-08T09:14:46.923154Z

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Observation 8a03da73-67dd-4a50-9d69-73d23e141473 · outbound

This paper cites 2: Strong alfvenic turbulence.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM 2: Strong alfvenic turbulence

Reference 6

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doi, observed 2026-07-08T09:14:46.917954Z

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Observation 29f79751-7f6a-4138-bde3-a748047103e0 · outbound

This paper cites Resolved magnetic dynamo action in the simulated intracluster medium.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Resolved magnetic dynamo action in the simulated intracluster medium

Reference 7

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local_arxiv, observed 2026-07-08T09:14:46.752687Z

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Observation bca77d02-e3e1-4d8c-8fa0-f1eb3431a24a · outbound

This paper cites Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence

Reference 8

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local_arxiv, observed 2026-07-08T09:14:46.841030Z

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Observation 7c2d7230-e984-4f96-85e0-c5827e0c7c36 · outbound

This paper cites Turbulent Heating in Galaxy Clusters Brightest in X-rays.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Turbulent Heating in Galaxy Clusters Brightest in X-rays

Reference 9

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local_arxiv, observed 2026-07-08T09:14:46.829375Z

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Observation 60d41de0-7927-4f23-9e9d-bb4740325dab · outbound

This paper cites Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

Reference 10

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local_arxiv, observed 2026-07-08T09:14:46.877103Z

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Observation 333e8010-d141-4911-8530-8a72a8dbbe55 · outbound

This paper cites The intracluster magnetic field power spectrum in Abell 2255.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The intracluster magnetic field power spectrum in Abell 2255

Reference 11

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local_arxiv, observed 2026-07-08T09:14:46.918893Z

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Observation ca60c768-d8cd-44d8-82af-f3450fcc6c49 · outbound

This paper cites Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi

Reference 12

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Observation a02ded75-3d59-4d1e-8e88-dc4d26fc9d4a · outbound

This paper cites XRISM forecast for the Coma cluster: stormy, with a steep power spectrum.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM XRISM forecast for the Coma cluster: stormy, with a steep power spectrum

Reference 13

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local_arxiv, observed 2026-07-08T09:14:46.900481Z

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Observation 2dd12ed8-db21-4fb1-bb31-be191fdc0151 · outbound

This paper cites The Radio Galaxy Messier 87 , year = 1999, editor =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The Radio Galaxy Messier 87 , year = 1999, editor =

Reference 14

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doi, observed 2026-07-08T09:14:46.885343Z

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Observation 68bb1b84-6a33-4540-af85-d19f83a540fb · outbound

This paper cites Cosmic rays and Radio Halos in galaxy clusters : new constraints from radio observations.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Cosmic rays and Radio Halos in galaxy clusters : new constraints from radio observations

Reference 15

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local_arxiv, observed 2026-07-08T09:14:46.881605Z

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Observation 2f73a27f-8aa9-4cf6-9f98-1edc08fd522a · outbound

This paper cites On the connection between turbulent motions and particle acceleration in galaxy clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM On the connection between turbulent motions and particle acceleration in galaxy clusters

Reference 16

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local_arxiv, observed 2026-07-08T09:14:46.802019Z

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Observation 1edc8a6e-b81d-4ef3-a7f1-03f331040a72 · outbound

This paper cites arXiv e-prints , keywords =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM arXiv e-prints , keywords =

Reference 17

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arxiv_id, observed 2026-07-08T09:14:46.818925Z

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Observation 430b38e4-d86b-4e3e-99f7-5dc99870f3d5 · outbound

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Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM eprint =

Reference 18

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arxiv_id, observed 2026-07-08T09:14:46.926294Z

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Observation a5b55b93-7ea0-4e6c-9964-2177c88efccf · outbound

This paper cites Cosmic rays in galaxy clusters and their non-thermal emission.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Cosmic rays in galaxy clusters and their non-thermal emission

Reference 19

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local_arxiv, observed 2026-07-08T09:14:46.778601Z

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Observation 7847675e-3265-4c36-b86e-fb7940ec7f45 · outbound

This paper cites A New Radio - X-Ray Probe of Galaxy Cluster Magnetic Fields.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM A New Radio - X-Ray Probe of Galaxy Cluster Magnetic Fields

Reference 20

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Observation e30c7fff-04fe-4b4e-b84d-fcc38fd6695b · outbound

This paper cites Rotation Measures of Radio Sources in Hot Galaxy Clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Rotation Measures of Radio Sources in Hot Galaxy Clusters

Reference 21

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local_arxiv, observed 2026-07-08T09:14:46.894896Z

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Observation 8ac6047d-31a3-4855-b0bd-1e27e2044976 · outbound

This paper cites Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs

Reference 22

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Observation 610784d6-5fd5-4dee-9549-96506f4f914f · outbound

This paper cites Faraday Rotation Measure Synthesis.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Faraday Rotation Measure Synthesis

Reference 23

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local_arxiv, observed 2026-07-08T09:14:46.755701Z

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Observation f363e160-edb6-4999-bc02-bb2bdeb84c4e · outbound

This paper cites Introduction to Faraday tomography and its future prospects.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Introduction to Faraday tomography and its future prospects

Reference 24

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local_arxiv, observed 2026-07-08T09:14:46.826710Z

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Observation c0307fcc-5106-4b3c-9e1f-96dddaeb9811 · outbound

This paper cites Probing the Magnetised Gas Distribution in Galaxy Groups and the Cosmic Web with POSSUM Faraday Rotation Measures.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Probing the Magnetised Gas Distribution in Galaxy Groups and the Cosmic Web with POSSUM Faraday Rotation Measures

Reference 25

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local_arxiv, observed 2026-07-08T09:14:46.930388Z

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

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Observation 27f776cc-b076-4418-b55d-8c9ca902e455 · outbound

This paper cites MHD Turbulence: A Biased Review.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM MHD Turbulence: A Biased Review

Reference 26

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local_arxiv, observed 2026-07-08T09:14:46.853169Z

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Observation 0e3e5a87-5c28-4e98-ab45-812b1131824b · outbound

This paper cites AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasma.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasma

Reference 27

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local_arxiv, observed 2026-07-08T09:14:46.875686Z

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.

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Observation 574f66b5-630a-4e9f-afe3-5ba1a86ee1f0 · outbound

This paper cites The Coma cluster magnetic field from Faraday rotation measures.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The Coma cluster magnetic field from Faraday rotation measures

Reference 28

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local_arxiv, observed 2026-07-08T09:14:46.828220Z

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.

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Observation a6207488-05dd-46c7-883a-d02a6e7b4f78 · outbound

This paper cites Sardinia Radio Telescope observations of Abell 194 - the intra-cluster magnetic field power spectrum.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Sardinia Radio Telescope observations of Abell 194 - the intra-cluster magnetic field power spectrum

Reference 29

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local_arxiv, observed 2026-07-08T09:14:46.908584Z

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.

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Observation c3202bed-046c-4535-941d-6aa7d44e3126 · outbound

This paper cites Suppressed effective viscosity in the bulk intergalactic plasma.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Suppressed effective viscosity in the bulk intergalactic plasma

Reference 30

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local_arxiv, observed 2026-07-08T09:14:46.871850Z

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.

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Observation 3f158738-3862-482f-a92f-f86ee6868c63 · outbound

This paper cites Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed with Chandra ACIS.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed with Chandra ACIS

Reference 31

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local_arxiv, observed 2026-07-08T09:14:46.842744Z

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.

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Observation c9a68e65-d1da-41ce-8647-1b1d611d29e6 · outbound

This paper cites Magnetic fields in the multiphase interstellar medium of the Milky Way: turbulent kinetic and magnetic energy density relation.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Magnetic fields in the multiphase interstellar medium of the Milky Way: turbulent kinetic and magnetic energy density relation

Reference 32

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local_arxiv, observed 2026-07-08T09:14:46.878482Z

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:e460991025401879c3e0148b39a2dbda028925bc288a8266c4ac3a7bf5fbcc78

Observation ac2b2d77-2f62-4f66-98b1-5bb9bc5aca12 · outbound

This paper cites Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis

Reference 33

Resolution
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local_arxiv, observed 2026-07-08T09:14:46.894387Z

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:e722d0e8a441ebb74413be5bef6975c9f3d2c94d6b7c7c2ee7b0183829eb54de

Observation fba22877-3191-48f8-88de-e289c1950ace · outbound

This paper cites MeerKAT view of the diffuse radio sources in Abell 3667 and their interactions with the thermal plasma.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM MeerKAT view of the diffuse radio sources in Abell 3667 and their interactions with the thermal plasma

Reference 34

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.869111Z

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=sha256:9b2df8b9439b427f2b9ad265baacae991f44694843f8b88fec41be3c379dd75d

Observation 90602f5f-7663-4373-9bf5-582a2073edc9 · outbound

This paper cites Galaxy clusters enveloped by vast volumes of relativistic electrons.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Galaxy clusters enveloped by vast volumes of relativistic electrons

Reference 35

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.797872Z

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=sha256:7dfb0f1dc81eb126ac834d0718b26bf88d643800c75143cab0b08599c996c88b

Observation 104c1e25-cc72-4273-a2a7-2548b999ffae · outbound

This paper cites A radio ridge connecting two galaxy clusters in a filament of the cosmic web.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM A radio ridge connecting two galaxy clusters in a filament of the cosmic web

Reference 36

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.874468Z

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=sha256:0603a06dd6444bdfcea353451942b2c67a1a1d4a59de56397d178293e6c757b0

Observation 9f44d36e-552c-49ac-b943-6f8361de0d46 · outbound

This paper cites Observations of a Pre-Merger Shock in Colliding Clusters of Galaxies.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Observations of a Pre-Merger Shock in Colliding Clusters of Galaxies

Reference 37

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.856241Z

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=sha256:71c9d48a23328c255df6a8cd581bede3251188210ca822cae795c8885a05dff5

Observation 30a03f72-293e-4883-ba86-99e1c0f82010 · outbound

This paper cites Diffuse radio source candidate in CIZA J1358.9-4750.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Diffuse radio source candidate in CIZA J1358.9-4750

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.920404Z

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:a1b04787628f49d0b2b0244d537845ac2341c44e2191508eb6d91cd9cb965a44

Observation 069d2dfd-3dec-4844-87b2-f02cfcc77a7d · outbound

This paper cites Second order Fermi reacceleration mechanisms and large scale synchrotron radio emission in intra-cluster bridges.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Second order Fermi reacceleration mechanisms and large scale synchrotron radio emission in intra-cluster bridges

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.940010Z

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:dabba215ac958b43bf89152e05b833a5265905feba00942e950a8d77aed4d8a6

Observation 3ba6ca66-da9d-44ef-93ce-a5fd7f9b13d2 · outbound

This paper cites Magnetism Science with the Square Kilometre Array.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Magnetism Science with the Square Kilometre Array

Reference 40

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.916339Z

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=sha256:59ee6a501e222ea09e33c36ae62e87bd0c294fc54736823d90c52237dbc28a55

Observation 5807c596-3865-4326-9254-7bbd9bd8fb53 · outbound

This paper cites Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.897443Z

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=sha256:4262a0855c542de64ea8bef08f9f43232c6f299b30d4f0ddbab4c3db0afba5e4

Observation 5941c1fd-dc49-4c95-bcaa-8d8dea4885c7 · outbound

This paper cites Structure functions with higher-order stencils as a probe to separate small- and large-scale magnetic fields.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Structure functions with higher-order stencils as a probe to separate small- and large-scale magnetic fields

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.882938Z

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=sha256:88d54459d1040fd18855f2e64d68aa7ec2cdf34f5b07520023f4e3cf2f1a54de

Observation 68582521-72b8-424f-ad4a-7e019b0fcce3 · outbound

This paper cites The Quiescent Intracluster Medium in the Core of the Perseus Cluster.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The Quiescent Intracluster Medium in the Core of the Perseus Cluster

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.888618Z

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:c385f05ea4541dd6ff59881488de5e7634ce544758cfae3ba200f74aaf7f840c

Observation ec9ab4b4-3c58-456c-92d7-30917436f1cf · outbound

This paper cites Dynamo theories.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Dynamo theories

Reference 44

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.911007Z

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=sha256:66297222870ed8130e74b733f32271b7000c1b9280bfb5e67e833ba1a181a3d8

Observation 5c46680d-44d8-4570-8992-3c966bbcbe4d · outbound

This paper cites , keywords =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM , keywords =

Reference 45

Resolution
verified exact
doi, observed 2026-07-08T09:14:46.920678Z

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=2026-07-08T09:12:09.993795Z digest=sha256:612cbddc5b813e24d197af34213bd5767b719a77c6522c4b64ce8ab9f0a8404c

Observation 62249a82-c1b1-4ce8-af7b-1ae92dd694ea · outbound

This paper cites Indications of an offset merger in Abell 3667.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Indications of an offset merger in Abell 3667

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.769083Z

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=sha256:001c2fb280cb156afcbf3c1743e8c4c01bc91a760efe892dcdd3ed5fa577c175

Observation 214e17c2-bf47-408f-81a0-93ddc1c65fec · outbound

This paper cites keywords =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM keywords =

Reference 47

Resolution
verified exact
doi, observed 2026-07-08T09:14:46.838206Z

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=2026-07-08T09:12:09.993795Z digest=sha256:db931d17b179c53516fbd8e1374d366115fa6619c674bee5feb90d2370812ad8

Observation cfd1ff4b-b0c9-4f34-a358-fd1df7998803 · outbound

This paper cites 2026, A&A, 705, A129, doi: 10.1051/0004-6361/202556070.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM 2026, A&A, 705, A129, doi: 10.1051/0004-6361/202556070

Reference 48

Resolution
verified exact
doi, observed 2026-07-08T09:14:46.933995Z

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=2026-07-08T09:12:09.993795Z digest=sha256:860f9d8921a0c878656e63531efe1c905a9a006be4942f00f2b18d0dcb92792b

Observation d536ad25-6b22-43ad-903d-638d1316a429 · outbound

This paper cites The bulk motion of gas in the core of the Centaurus galaxy cluster.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The bulk motion of gas in the core of the Centaurus galaxy cluster

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.937012Z

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=sha256:4ae8d16b387b62afcd0e73f5f18575cfa873e6dffdb7a39e2e1b98df8f255084

Observation 91eeee5c-ca18-465c-a847-570707beb252 · outbound

This paper cites , keywords =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM , keywords =

Reference 50

Resolution
verified exact
doi, observed 2026-07-08T09:14:46.913253Z

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=2026-07-08T09:12:09.993795Z digest=sha256:6f4742ec15d1e45ae4892d12f4d43061119fde81012a081830063052aea82c0f

Observation 8f5a2090-bdc0-46de-9895-fb0ac289ac85 · outbound

This paper cites The relation between gas density and velocity power spectra in galaxy clusters: high-resolution hydrodynamic simulations and the role of conduction.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The relation between gas density and velocity power spectra in galaxy clusters: high-resolution hydrodynamic simulations and the role of conduction

Reference 51

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.906926Z

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=sha256:6373310489eec35637a34d58f8571787f909b87c05b66a7252b42f4bd5e0ffca

Observation 030a6949-1b2e-49b1-bed0-a9f7b1240105 · outbound

This paper cites Gas Perturbations in Hot Smooth Atmospheres X-ray Surface Brightness Fluctuations in Smooth Galaxy Cluster Atmospheres.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Gas Perturbations in Hot Smooth Atmospheres X-ray Surface Brightness Fluctuations in Smooth Galaxy Cluster Atmospheres

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.820158Z

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:befaa5719f2d71b9164a7400716982f297bd96f9453d80d789ac9ef61e6e2c48

Observation 594b8e04-cdf5-415d-a5a5-5b83b5a2146d · outbound

This paper cites A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417

Reference 53

Resolution
metadata mismatch
arxiv_id, observed 2026-07-08T09:14:46.816658Z

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=2026-07-08T09:12:09.993795Z digest=sha256:34ce60ff7d45e8a96f252b837dd42aba102a56fd002329569c6309510eb41e66

Observation c75522a0-974e-4463-8866-15058ba0c775 · outbound

This paper cites Unexpected Circular Radio Objects at High Galactic Latitude.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Unexpected Circular Radio Objects at High Galactic Latitude

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.837438Z

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=sha256:1a0582ca0835a1150a305d762ae353b66946d0b9bdfd75e02c94a1c54fc1b864

Observation 3f73953e-7c63-4b6d-9d65-7cedc0dcb449 · outbound

This paper cites Single- and double-headed odd radio circles in the LOFAR surveys.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Single- and double-headed odd radio circles in the LOFAR surveys

Reference 55

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.862164Z

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=2026-07-08T09:12:09.993795Z digest=sha256:200e42de2bdc0721c46acbd1288ad2a3216a19a59be62e44d5ad6526e114ea91

Observation 8637c636-cc4b-4e36-917e-2df9446ca35e · outbound

This paper cites Discovery of Diffuse Radio Source in Abell 1060.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Discovery of Diffuse Radio Source in Abell 1060

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.850613Z

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:cfb268f14b62f6bb65d23d185e4eee36086b26395dcd76271abb2cb352612f8f

Observation a8480530-8b34-44ef-8990-5f836fb59286 · outbound

This paper cites year = 1968, month = jan, volume =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM year = 1968, month = jan, volume =

Reference 57

Resolution
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doi, observed 2026-07-08T09:14:46.896865Z

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=2026-07-08T09:12:09.993795Z digest=sha256:a19123de18c7df47383479c5eb21c3497732d833ae3c27d91c4f86e786f8d062

Observation 9f32c2a3-2dc3-4f1b-8455-a396fb7b5fbf · outbound

This paper cites , keywords =.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM , keywords =

Reference 58

Resolution
verified exact
doi, observed 2026-07-08T09:14:46.922932Z

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=2026-07-08T09:12:09.993795Z digest=sha256:2fe8516577f14619c7aa18b53ee4ec34b56c2b644d3970684dd68ca7086021b9

Observation b9240cbc-1d73-4f35-b6fe-eb1924ba9b97 · outbound

This paper cites Merger-driven multi-scale ICM density perturbations: testing cosmological simulations and constraining plasma physics.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Merger-driven multi-scale ICM density perturbations: testing cosmological simulations and constraining plasma physics

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.822147Z

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=sha256:8a54df510159bc2ee8987d15e62b30d4287a3fa5dbfa844bc78eb6a9d3bd583e

Observation 48c3d0e0-0314-4666-8148-cbc0f383320e · outbound

This paper cites Magnetic fields and relativistic electrons fill entire galaxy cluster.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Magnetic fields and relativistic electrons fill entire galaxy cluster

Reference 60

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.754387Z

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=sha256:71b3722530cc5e2a260c3a97209b81082b3a5d66d293ab989b2823f2572c7628

Observation 8407dbaf-eb1f-4606-9fed-c40a114828ef · outbound

This paper cites Stochastic reacceleration of relativistic electrons by turbulent reconnection: a mechanism for cluster-scale radio emission ?.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Stochastic reacceleration of relativistic electrons by turbulent reconnection: a mechanism for cluster-scale radio emission ?

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.950577Z

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=sha256:140d2109e6a2e1e6ea1b188b1fbccd26675e5fcf50554fe9e98304d4c627ced5

Observation 7c436aac-74f3-4c6d-9db6-a14f6015c767 · outbound

This paper cites The diffuse radio emission from the Coma cluster at 2.675 GHz and 4.85 GHz.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The diffuse radio emission from the Coma cluster at 2.675 GHz and 4.85 GHz

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.934229Z

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:e3ebab56f8b8f02443645a53ae11a72ad41b4b7b1e4fa302190c9fa5647ffbbc

Observation 0e9268a2-714c-4b7c-9f08-727df5d5b74a · outbound

This paper cites Turbulence and Magnetic Fields in the Large Scale Structure of the Universe.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Turbulence and Magnetic Fields in the Large Scale Structure of the Universe

Reference 63

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.902722Z

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:d04f3a855d2a0d41f66a169441f5d04bead07f4dfcd669f60dd9c732a070e609

Observation b2bb3ae5-95e5-4199-afd3-81d6f28b14ad · outbound

This paper cites Faraday Rotation Measure due to the Intergalactic Magnetic Field.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Faraday Rotation Measure due to the Intergalactic Magnetic Field

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.769937Z

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:cea2388087ba0daf493d22207fd812f9b7d415a6ba02d99a5e4be0e6ef498392

Observation 8a52c9c5-d3ec-487b-8cfc-49818c1a0e27 · outbound

This paper cites Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters

Reference 65

Resolution
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local_arxiv, observed 2026-07-08T09:14:46.936765Z

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:c1e545204f56ae28503d36a36104454902c6a1e57b3f0a0e59a670a84a9905e1

Observation 9266e3a4-95c5-48d4-b6be-7f0f83b65f7d · outbound

This paper cites Shukurov and K.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Shukurov and K

Reference 66

Resolution
metadata mismatch
doi, observed 2026-07-08T09:14:46.864627Z

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=2026-07-08T09:12:09.993795Z digest=sha256:2e1dea43158dba133962996e3645b7b398a420a073d274695e94f113e3d2da73

Observation 96bbaf95-56da-49f6-b997-474c79f4a962 · outbound

This paper cites Diffuse Radio Emission from Galaxy Clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Diffuse Radio Emission from Galaxy Clusters

Reference 67

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.736052Z

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:fcc0633efdb23184c8c7cb97a4e418f43ffb89d505485ed38658d7660186c14a

Observation 9bc46739-7759-4e84-8c7d-919e53e76bfd · outbound

This paper cites Probing Turbulence in the Coma Galaxy Cluster.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Probing Turbulence in the Coma Galaxy Cluster

Reference 68

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.942770Z

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=sha256:444a0766aa4b872e4c61f81532920c38cdc13d3f4b4026e7f7d447dae33fc879

Observation 24f77766-cd29-410b-a9be-c546caf8a335 · outbound

This paper cites Turbulence and Magnetic Fields in Astrophysical Plasmas.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Turbulence and Magnetic Fields in Astrophysical Plasmas

Reference 69

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.810391Z

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=2026-07-08T09:12:09.993795Z digest=sha256:611de51e50be1dc5007ff9f8852f42e58377b37a805729e0b58f8dc28cd60eb0

Observation b43d6007-e817-4c60-bfd5-63e9ca306e8a · outbound

This paper cites Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.845275Z

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=sha256:617bc98737c6a33f1d2dc3e735c7eb3162b2c40ba44bfcb99df8825181b005ca

Observation a5e36f83-4a27-446d-9679-792cd6827efb · outbound

This paper cites Suppression of small scale dynamo action by an imposed magnetic field.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Suppression of small scale dynamo action by an imposed magnetic field

Reference 71

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.953143Z

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:ada0b5ee36e4c1243187ed75c2fa787eafa4b884be282f3a7799b72d8d3f5cd6

Observation df6c1d1d-07eb-4d1d-b755-510a179f2f9e · outbound

This paper cites Simulations of small-scale turbulent dynamo.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Simulations of small-scale turbulent dynamo

Reference 72

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.955921Z

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=sha256:18849f93c4abb973036cd4d3699927a63222e3cbf493efc31d3f254bc2eb9e2e

Observation 280626f2-989f-46b6-9db7-1a53f2c95a7b · outbound

This paper cites and Yang , J.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM and Yang , J

Reference 73

Resolution
metadata mismatch
arxiv_id, observed 2026-07-08T09:14:46.840020Z

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=2026-07-08T09:12:09.993795Z digest=sha256:2e1ea1635e2b0c03bc734ebb47871c16aa92480709e07a49966d1e81a0ab4f8c

Observation 2a05ffb0-1e2b-408b-a345-10167d54750f · outbound

This paper cites Seed magnetic fields in turbulent small-scale dynamos.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Seed magnetic fields in turbulent small-scale dynamos

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.925561Z

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=sha256:9d215fe502acb45a34f7208b7dba7d2ddcde6026759c84c8deaeeed726202e0e

Observation b61c9d18-42d9-462f-99ea-5fbe3e5e7c74 · outbound

This paper cites The origin, evolution and signatures of primordial magnetic fields.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The origin, evolution and signatures of primordial magnetic fields

Reference 75

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.909612Z

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=sha256:27cf4a29e4edd4c782d30a7dfc138fc7870b44cab77104b6364427894b5120c4

Observation ba41c5f0-9be9-46dd-9b24-1682a98f9964 · outbound

This paper cites On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM On the saturation mechanism of the fluctuation dynamo at ${\text{Pr}_\mathrm{M}} \ge 1$

Reference 76

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.928540Z

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=sha256:0d885a511c5b41d6abde61a94bc3bd183d914e5eef92c52a8d356d290870826b

Observation 761194ac-4206-4abf-8e42-ba255513bd3f · outbound

This paper cites Turbulent Amplification and Structure of the Intracluster Magnetic Field.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Turbulent Amplification and Structure of the Intracluster Magnetic Field

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.785091Z

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=sha256:36cd8322263332d3b31d9b93a2cd3a4fc8dea57c2abdb4de5654803ec4dfa88d

Observation 694f4c73-cf14-4ef5-b22c-bd48502a7893 · outbound

This paper cites Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas

Reference 78

Resolution
metadata mismatch
local_arxiv, observed 2026-07-08T09:14:46.945402Z

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=sha256:8194f3b827b0c7705de2278b4b08a4d4c49591f15fcf303a17b9f98e376bafb1

Observation bb12b2d2-9b2b-4f7c-a1d8-6afa4a4b2f35 · outbound

This paper cites Fluctuation dynamos and their Faraday rotation signatures.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Fluctuation dynamos and their Faraday rotation signatures

Reference 79

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.791222Z

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=sha256:57410d752e01179d80337d916db16211137d9e36980b2f9227b1bbc9b134f91f

Observation b5380196-d083-499a-a64e-848fad2d12b9 · outbound

This paper cites Probing cluster magnetism with embedded and background radio sources in Planck clusters.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM Probing cluster magnetism with embedded and background radio sources in Planck clusters

Reference 80

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.915557Z

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:a0a4cb03332a39bc3e195777a75dc049a0493788d4ffe5905edfa2ae9af848cd

Observation dc37bba7-e6a1-4206-b56d-f8fd1a9b01f9 · outbound

This paper cites The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems.

Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:14:46.731161Z

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=2026-07-08T09:12:09.993795Z digest=sha256:49a8a612e8823ebbcd401e83d31c68a51497481bc3f669caaa12c446772a3187

Pith citing papers

No inbound Pith citation observations are available.