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First results from the IllustrisTNG simulations: radio haloes and magnetic fields

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 58 inbound Pith citation observations for arXiv:1707.03396.

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pith.paper-citation-record.v1
1707.03396 v2

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measured 58 of 58 standing notices

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measured 58 of 58 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:06:27.176119Z

measured 1 of 1 external citation measurements

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Source: pith, observed 2026-07-10T18:07:31.339015Z

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Pith citing papers

Observation cf418287-6a8c-4c08-831a-06937c9bafe7 · inbound

First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback cites this paper.

First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 295

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Observation d28ef9ab-5dd8-4f0c-9338-ea8c7203c73b · inbound

The impact of cosmic filaments on the abundance of satellite galaxies cites this paper.

The impact of cosmic filaments on the abundance of satellite galaxies First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 38

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Observation bb9572ab-15eb-4064-b6db-f26ef4be0bd5 · inbound

Cavendish experiment with fast radio bursts on cosmological scales cites this paper.

Cavendish experiment with fast radio bursts on cosmological scales First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 75

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Observation 5d42ff2c-b489-4a0c-ac58-94fad33cf8ed · inbound

Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum cites this paper.

Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 34

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The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles cites this paper.

The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 53

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Observation 81770935-70ac-4e9c-a7b8-4e27e7dfcc01 · inbound

Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy cites this paper.

Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 105

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Observation 37cfddba-7337-4868-99fa-6b1d37579e3b · inbound

Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations cites this paper.

Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 35

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Observation 37004774-d7b1-417b-8fe1-7ecdcbe7e433 · inbound

Understanding the regulation of star formation within TNG100 galaxies on kpc-scales using machine learning I: Global versus local cites this paper.

Understanding the regulation of star formation within TNG100 galaxies on kpc-scales using machine learning I: Global versus local First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 11

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Observation 77f34b2d-e684-4137-aadd-71e055b1f067 · inbound

Classifying Supermassive Black Hole Growth Regimes to Observables Across Cosmological Simulations with Forecasts for LSST cites this paper.

Classifying Supermassive Black Hole Growth Regimes to Observables Across Cosmological Simulations with Forecasts for LSST First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 32

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Observation 854f62ee-c7f3-4032-b9c9-0f5e10b02df6 · inbound

Galaxy Populations in the IllustrisTNG Caustic Skeleton cites this paper.

Galaxy Populations in the IllustrisTNG Caustic Skeleton First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 128

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Observation d75b105d-f959-4ba1-bad4-7b0590a14ddb · inbound

Cosmological constraints from the small scale clustering of Emission Line Galaxies cites this paper.

Cosmological constraints from the small scale clustering of Emission Line Galaxies First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 181

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Observation f584e44d-120c-484d-9585-a25e2da3a1a3 · inbound

Dynamically cold discs in high-redshift galaxies: comparison between ALMA observations and TNG50 cites this paper.

Dynamically cold discs in high-redshift galaxies: comparison between ALMA observations and TNG50 First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 42

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Observation 1c4a9eb2-c5fa-427c-a21d-c3313a98f439 · inbound

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation cites this paper.

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 24

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Observation baa0f511-914b-416c-9c65-8dd59c22735c · inbound

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation cites this paper.

Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 24

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Observation be609231-0f3f-42cb-b457-e18c7332ec37 · inbound

The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model cites this paper.

The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 47

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Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos cites this paper.

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 59

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The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries cites this paper.

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 143

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Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations cites this paper.

Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 171

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A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies cites this paper.

A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 69

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Dynamical evolution of Milky Way globular clusters on the cosmological timescale II. Terzan 2, 4, and 5 mass loss and collision tracking cites this paper.

Dynamical evolution of Milky Way globular clusters on the cosmological timescale II. Terzan 2, 4, and 5 mass loss and collision tracking First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 78

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Observation b17d658f-0545-459b-b1e7-e36a87f86f12 · inbound

Identification of Compact Groups of Galaxies in IllustrisTNG300 cites this paper.

Identification of Compact Groups of Galaxies in IllustrisTNG300 First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 27

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First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe cites this paper.

First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 93

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Probing the faint end of simulated galaxy counts at z>3 cites this paper.

Probing the faint end of simulated galaxy counts at z>3 First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 6

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Observation cf279d9a-31d8-4d89-80e2-99e4eaebea56 · inbound

Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues cites this paper.

Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 57

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\texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series cites this paper.

\texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 188

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Observation 2e361345-430f-498e-b3d8-e1942d9daabe · inbound

A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones cites this paper.

A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 50

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Observation f5ac1074-2471-4784-bc80-00d0d1f2ffca · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 113

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Observation f16fc452-2c26-493d-921d-c3db125afbf1 · inbound

TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates cites this paper.

TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 147

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Observation c8c7a1a6-9ac5-476b-8f09-b7d586eb650d · inbound

A Measurement of the Thermal and Ionization State of the IGM at $z < 0.5$ cites this paper.

A Measurement of the Thermal and Ionization State of the IGM at $z < 0.5$ First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 148

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Observation c93f8640-1ade-46e3-8c1e-7b0a502c8a18 · inbound

Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster cites this paper.

Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 98

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Observation 8e9440fc-04e8-4d07-b3c6-0a8d1e2f08d5 · inbound

A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst cites this paper.

A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 195

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verified exact
local_arxiv, observed 2026-06-27T21:51:19.039383Z

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Observation acb61b4e-72ef-4ae1-a95b-0a376b019ce2 · inbound

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 151

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verified exact
local_arxiv, observed 2026-06-27T16:11:02.277924Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:37a89f85b1e333e5a06bd1aabb9e36b465513860b2553e39f515583621d46db8

Observation b4a6568b-5068-4971-b177-9fcb42da672a · inbound

A universal model for the accretion rates and formation times of dark matter halos cites this paper.

A universal model for the accretion rates and formation times of dark matter halos First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 64

Resolution
verified exact
doi, observed 2026-06-27T15:41:01.388263Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-27T15:34:25.812471Z digest=sha256:74765235c07a7a7df4d65c1162c778bc7b990e0e489f256bd9881b54113bd83d

Observation cb5e58e2-10ad-4b23-a06f-5383f03495ed · inbound

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations cites this paper.

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-06-27T16:01:02.087999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:21c0614f59d42c8c37443c27e2bb5d2ada080e7a914ba5c6a6d48f20b3beaead

Observation 535dddc2-c06c-4ab3-b9e9-e20d59707518 · inbound

Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures cites this paper.

Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:21:00.339652Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c6f163e9e1cb1bff47599b7830d9ba7bce6f9731d746f2945ae6ae154b92a708

Observation 3a4a7b8c-0a16-42d9-8b57-68c0119e01f7 · inbound

Learning the Universe with the 2nd Generation of CAMELS: Varying 35 parameters of the IllustrisTNG model in (50Mpc/h)^3 boxes cites this paper.

Learning the Universe with the 2nd Generation of CAMELS: Varying 35 parameters of the IllustrisTNG model in (50Mpc/h)^3 boxes First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 47

Resolution
verified exact
doi, observed 2026-06-27T19:31:11.088739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-27T15:13:34.548481Z digest=sha256:8aff116cec2dc85da17fabeffbfed36c37be23cb024a61be0ca745f703dde566

Observation 12bec358-2f97-46a9-9a91-6dd94a743dd8 · inbound

Exploring the Relationship Between Bars, Star Formation Activity, and Host Galaxy Properties from $\mathbf{z \sim 0}$ to $\mathbf{z \sim 2}$ cites this paper.

Exploring the Relationship Between Bars, Star Formation Activity, and Host Galaxy Properties from $\mathbf{z \sim 0}$ to $\mathbf{z \sim 2}$ First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 85

Resolution
metadata mismatch
doi, observed 2026-06-27T03:00:24.126223Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-27T02:58:35.061370Z digest=sha256:61e214d017dc65e16765633dd4e41b6edad0a648359fbd4562910a25b3f0ae35

Observation ef3fa745-ab3a-4475-9391-ee9e69f7476c · inbound

TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation cites this paper.

TNG SAM: Bridging Hydrodynamical Complexity and Semi-Analytic Efficiency to Model Galaxy Formation First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 79

Resolution
verified exact
doi, observed 2026-06-27T00:30:17.034205Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T23:41:20.418211Z digest=sha256:011b6643c3c1177a8b0c7ac872d193c5eb34814dd2181e9751f01e5645ee36bc

Observation f1886cf5-22fa-4a1e-b702-12922e195151 · inbound

A Consistent Comparison of Intracluster Light Assembly in Simulations I. Redshift Evolution and Progenitor Galaxies cites this paper.

A Consistent Comparison of Intracluster Light Assembly in Simulations I. Redshift Evolution and Progenitor Galaxies First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 6

Resolution
verified exact
local_arxiv, observed 2026-06-26T16:59:36.151017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ba2787fdba483d81f4adea9df2de5d2871296f91aa0e129bd1d5e4decba48b05

Observation 1f6e6c4c-b592-420b-9daa-b2a5cb621c93 · inbound

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters cites this paper.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 172

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:59:08.475491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:054b07b338efa6c3841a68f696a0af473518290dbe6caa376160fb29ea52b3c5

Observation a998cad8-db10-44b8-a81f-7d43ce4961a6 · inbound

Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos cites this paper.

Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 35

Resolution
metadata mismatch
doi, observed 2026-06-25T23:58:42.795037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-25T23:52:21.029726Z digest=sha256:fcaf6aa14cf20cbf9454b1489d0ab36fdcb831512d8957c08c11ba49801b4eb9

Observation 0704e1cd-a20e-4970-919a-ac1ed0445bf9 · inbound

The dependence of Circumgalactic Medium properties on halo assembly histories in the IllustrisTNG simulations cites this paper.

The dependence of Circumgalactic Medium properties on halo assembly histories in the IllustrisTNG simulations First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 39

Resolution
metadata mismatch
doi, observed 2026-06-25T23:38:41.891626Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-25T23:31:31.386812Z digest=sha256:e99926c60e74409f5fbd720105bf5f618c809ce6171fa3b201931ff672f365be

Observation fb1684e0-99e3-4241-8210-7081ad4540ea · inbound

A Stellar Role Reversal: Multiple Features in the Mass and Mass Ratio Distributions of Merging Binary Black Holes from Stable Mass Transfer cites this paper.

A Stellar Role Reversal: Multiple Features in the Mass and Mass Ratio Distributions of Merging Binary Black Holes from Stable Mass Transfer First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 56

Resolution
metadata mismatch
doi, observed 2026-06-26T06:39:04.650787Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-26T01:19:48.682397Z digest=sha256:1620e840620b6c8913e3e658ee9ecf07d38673ed7b4b737a876d064bc098bb89

Observation be5f299b-0ea5-4fcf-b7d8-483ab81f5d31 · inbound

Forward-modelling the Tolman and distance-duality tests with IllustrisTNG cites this paper.

Forward-modelling the Tolman and distance-duality tests with IllustrisTNG First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 26

Resolution
verified exact
doi, observed 2026-06-26T03:58:57.546649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T03:52:24.934567Z digest=sha256:d0144a004a1a51aa477a703d036e3a5758176377cb2cd3ea21e6e92cb954316f

Observation 059f171d-046f-4017-a9e1-b94e1c4d4856 · inbound

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec cites this paper.

MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 245

Resolution
verified exact
local_arxiv, observed 2026-06-29T04:03:05.560211Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2e204002109eb5c52255ccef86c212a9581c85256ea9dff5b3a80e2d5b4c22e7

Observation 5c4bbb6f-8729-416a-92b9-10d8c939e980 · inbound

The effect of dark energy on the void-halo perpendicular alignments cites this paper.

The effect of dark energy on the void-halo perpendicular alignments First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 3

Resolution
verified exact
local_arxiv, observed 2026-06-29T03:23:05.082204Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:dbdae3592ee93448a17fe0dd7a34f37faba90f96213a9b9e832ef92cd38c3c98

Observation ac200a20-32a1-412b-b9f6-78c08f453d0f · inbound

The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models cites this paper.

The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 208

Resolution
verified exact
local_arxiv, observed 2026-06-30T05:04:19.627379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:525803d84c86d06787904dee29771c30b2647554f600a24e7667f77c2304a87a

Observation fc999d55-5552-4ac8-9ff5-e672efb05775 · inbound

Optically Selected Superthin Galaxies Remain Thin in the Near-infrared cites this paper.

Optically Selected Superthin Galaxies Remain Thin in the Near-infrared First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 6

Resolution
verified exact
local_arxiv, observed 2026-07-02T09:36:48.876228Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:160064f48d3f515c491eddc5f877eaa20400c1bca88d09aa1b551e568fac2185

Observation 7550e4de-e2f8-4111-adea-b204061babae · inbound

Cosmology from HI galaxy surveys with the SKA cites this paper.

Cosmology from HI galaxy surveys with the SKA First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-07-02T06:46:44.201682Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e2794b920cc06c817f3d93e1cbd8c202ffe240753d134e0625ec0b895eea8ad9

Observation 8f7fa541-5bc0-4dde-9314-faeae414e42e · inbound

Constructing a Mock Galaxy Catalog for the All-sky SPECtroscopic Survey of Nearby Galaxies (A-SPEC) Using the Machine-assisted Semi-Simulation Model cites this paper.

Constructing a Mock Galaxy Catalog for the All-sky SPECtroscopic Survey of Nearby Galaxies (A-SPEC) Using the Machine-assisted Semi-Simulation Model First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 83

Resolution
metadata mismatch
doi, observed 2026-07-09T22:56:37.542495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-07-09T22:50:50.117291Z digest=sha256:dbd93dec4aadda9b66658f908904c74de72de54917f9a6b196211b73b8168068

Observation 9ca33993-9458-4825-ae0f-a7055891d6f5 · inbound

Tracing black hole and galaxy growth across environments since cosmic noon cites this paper.

Tracing black hole and galaxy growth across environments since cosmic noon First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-07-10T18:07:31.340717Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d24b78f175485f1e87bd1a027bfecdb5d28f94ccf0c9e24f0a0a50bf375da683

Observation f244c841-a45c-4b53-a717-a78b78dccfa6 · inbound

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods cites this paper.

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 35

Resolution
unresolved
no resolver link, observed 2026-07-13T04:41:12.165957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T04:41:12.165957Z digest=sha256:4fcc15cb1a31c13de04a57110045e9608faa7a9eecb776d22a0084ee74efcf35

Observation a5049ba2-cb40-48dd-bd51-b94a5fd6efe5 · inbound

Simulation-Based Priors for HI Bias from Halo Occupation Physics cites this paper.

Simulation-Based Priors for HI Bias from Halo Occupation Physics First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-02T02:52:36.021305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T02:52:36.021305Z digest=sha256:d71cf052657642a8e0e1395fc33514bd4656c2c63f6d94669cb2600ac6c21e57

Observation be284beb-d258-4ae5-9194-0970a1945d5b · inbound

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 173

Resolution
unresolved
no resolver link, observed 2026-08-02T00:50:15.491964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:50:15.491964Z digest=sha256:34392d13ac42fb09bc145479f1b6c148f020733d5e44ea85c5c84c170ff3db15

Observation 9d5c6a5a-e8f4-4846-89d1-3a13cdf8a8a7 · inbound

The role of filaments in the large-scale conformity signal cites this paper.

The role of filaments in the large-scale conformity signal First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-01T04:25:28.565762Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T04:25:28.565762Z digest=sha256:b051ee312a36c03da6d86ac699ca54481d9709ee235707513457a7b864116ac8

Observation 57b0c99f-3761-4f36-8b3c-56cf3f22cd38 · inbound

Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe cites this paper.

Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 185

Resolution
unresolved
no resolver link, observed 2026-08-01T00:56:22.046879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:56:22.046879Z digest=sha256:f34ef538e6bc4710d31472ada56fc6af9e844d8c2c534046b66fcda2113392cf

Observation 2814a703-d124-4ef0-b451-e2c698c866fa · inbound

High-mass binary black hole mergers from detailed binary evolution models cites this paper.

High-mass binary black hole mergers from detailed binary evolution models First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 80

Resolution
unresolved
no resolver link, observed 2026-07-31T22:07:32.538702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T22:07:32.538702Z digest=sha256:0bba3b756ae1010d3dc825680f6ed4cc275d289c14dc51657ecf9ccd5b14aa02

Observation 4243abba-3fd5-4103-94e1-86f68d98d3d0 · 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 First results from the IllustrisTNG simulations: radio haloes and magnetic fields

Reference 149

Resolution
unresolved
no resolver link, observed 2026-08-06T00:06:27.176119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T00:06:27.176119Z digest=sha256:4731467e1394cc89c0e5feb82fbce65ac616f96d3c4b6ab51091e79b14a3d3f6