Paper Citation Record · LEDGER

First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:1902.05553.

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pith.paper-citation-record.v1
1902.05553 v2

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measured 16 of 16 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:53:26.729465Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-07T17:24:00.761242Z

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Outbound references

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Pith citing papers

Observation 3401d711-e50e-41e6-857e-bad1116bdeb1 · inbound

The buildup of strongly barred galaxies in the TNG100 simulation cites this paper.

The buildup of strongly barred galaxies in the TNG100 simulation First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-14T15:53:26.729465Z

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Unavailable: canonical work link unavailable.

Observation 588bbd9e-d8a0-461f-8135-041f9b8c399a · inbound

The Formation of Ultra-Diffuse Galaxies in the RomulusC Galaxy Cluster Simulation cites this paper.

The Formation of Ultra-Diffuse Galaxies in the RomulusC Galaxy Cluster Simulation First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-14T13:11:33.823720Z

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Observation 248e8fbc-d21e-44cd-b567-f9de5228427a · inbound

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level cites this paper.

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-12T00:58:57.597522Z

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Observation fb4ccc8f-8ddd-4b8b-8973-5fb4a17b2321 · inbound

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations cites this paper.

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T14:57:14.203258Z

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Observation 3367f044-af52-4cc4-8750-bca46af58ffc · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 230

Resolution: unresolved; no resolver link, observed 2026-08-06T18:16:14.542762Z

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Observation f2a8dcb5-5c00-4fad-a7cb-fa0003ec93a8 · inbound

Axion lines from nuclear de-excitations in galactic stellar populations cites this paper.

Axion lines from nuclear de-excitations in galactic stellar populations First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:49.447999Z

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Observation b8f84e7f-e2f8-4a7e-a574-1e45d8270474 · inbound

The History of Galaxy Mergers in IllustrisTNG cites this paper.

The History of Galaxy Mergers in IllustrisTNG First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-04T19:17:16.681831Z

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Unavailable: canonical work link unavailable.

Observation c811db5c-a8fe-4067-886c-17a80c74bc93 · 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 TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-02T17:14:02.704052Z

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Unavailable: canonical work link unavailable.

Observation 242a520f-c3f9-4816-aea5-58cd11729494 · inbound

Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years cites this paper.

Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 94

Resolution: verified exact; local_arxiv, observed 2026-07-07T17:24:00.763515Z

Source-reported events for the cited work

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Observation 296ac36e-e6c2-4574-b10c-e4d7060c6423 · inbound

Turbulent Transport of Galactic Magnetic Fields into Cosmic Voids: Insights from IllustrisTNG cites this paper.

Turbulent Transport of Galactic Magnetic Fields into Cosmic Voids: Insights from IllustrisTNG First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 21

Resolution: unresolved; no resolver link, observed 2026-07-13T02:42:00.655584Z

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Observation beaa0a82-be31-45f7-9c00-63a24e2a6cbe · inbound

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 107

Resolution: unresolved; no resolver link, observed 2026-08-02T03:50:11.699968Z

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Observation cdb05275-d902-45cc-a6c1-66bb3dad10bf · 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 TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 167

Resolution: unresolved; no resolver link, observed 2026-08-02T00:50:15.464381Z

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Observation 7b51be3c-0632-4150-8112-41a3b6ebbd9e · inbound

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters cites this paper.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-01T23:43:55.787920Z

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Unavailable: canonical work link unavailable.

Observation 1561b954-91a7-415d-a0d9-2d2cfb34a8a9 · inbound

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba cites this paper.

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 262

Resolution: unresolved; no resolver link, observed 2026-08-01T08:26:28.237365Z

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Unavailable: canonical work link unavailable.

Observation 1058c616-89ae-4d9d-af26-6acf1f48916a · inbound

Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection cites this paper.

Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-04T01:15:11.436934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88ab87b0-63d0-4061-8e15-f2625b7db154 · inbound

The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data cites this paper.

The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-12T00:16:22.884201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.