First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies | Paper Citation Record

Observation 2b18132e-d71f-4952-8fef-09de91e41287 · inbound

Realistic simulations of galaxy formation in f(R) modified gravity cites this paper.

Realistic simulations of galaxy formation in f(R) modified gravity First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-05-25T02:00:12.385120Z

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Observation 50c30b9c-9b34-4f7b-abf8-f9a7a11c8b5b · inbound

De-baryonifying halos via optimal transport cites this paper.

De-baryonifying halos via optimal transport First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-12T11:18:48.358804Z

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Observation 0097522f-3ced-42a8-b2c3-dcfa42db5e81 · inbound

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data cites this paper.

Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 94

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Observation d521dace-4af7-4516-922d-f4e2eb1a8719 · inbound

The Optical and Infrared Are Connected cites this paper.

The Optical and Infrared Are Connected First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 2

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Observation 6cd8d673-b472-473d-912b-63c85eedf81b · inbound

Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog cites this paper.

Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 64

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Observation 37c3503c-0be5-42e5-82b8-34807bc9804c · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 229

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Observation c1a9408d-d131-461d-8d95-0c6356c1befa · inbound

Missing baryons recovered: a measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel'dovich effect and CMB lensing cites this paper.

Missing baryons recovered: a measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel'dovich effect and CMB lensing First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-06T16:15:52.817485Z

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Observation 64bd5f1b-c44b-4416-adc5-f0fcd9ddf544 · 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: the stellar mass content of groups and clusters of galaxies

Reference 44

Resolution: metadata mismatch; doi, observed 2026-05-18T12:56:24.072849Z

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Observation 5e047be8-f4f1-4235-93b4-de8b30aa2c15 · 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: the stellar mass content of groups and clusters of galaxies

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-03T22:28:30.658923Z

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Observation e144cfd8-dda4-4662-986e-ab2c6885c018 · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 71

Resolution: metadata mismatch; doi, observed 2026-05-17T01:58:51.117206Z

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Observation 1ebe2938-7561-43d4-a3cb-36d3348b46f4 · inbound

Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations cites this paper.

Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 115

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Observation b825ea24-7a0b-4b4d-828d-8d780333c3d9 · inbound

Galaxy discs regulate the growth of supermassive black holes cites this paper.

Galaxy discs regulate the growth of supermassive black holes First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 64

Resolution: verified exact; doi, observed 2026-05-10T18:20:41.992724Z

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Observation 1628886c-ba72-47b4-a497-eb0fb6647cf1 · inbound

Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario cites this paper.

Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 73

Resolution: verified exact; arxiv_id, observed 2026-05-11T08:00:58.895368Z

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Observation e7bd5a0e-cd81-40fa-8dfa-9829b82ca08c · 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: the stellar mass content of groups and clusters of galaxies

Reference 56

Resolution: metadata mismatch; doi, observed 2026-05-10T16:05:34.275517Z

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Observation 973b325b-3446-43f6-9716-079a740750e4 · inbound

Galaxy Populations in the IllustrisTNG Caustic Skeleton cites this paper.

Galaxy Populations in the IllustrisTNG Caustic Skeleton First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 154

Resolution: metadata mismatch; doi, observed 2026-05-10T03:54:36.638903Z

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Observation 1eae5321-c25c-4f28-9808-366bfce70aae · inbound

Analysis of synthetic OVI absorption associated with galaxy groups in SIMBA and TNG50 simulations cites this paper.

Analysis of synthetic OVI absorption associated with galaxy groups in SIMBA and TNG50 simulations First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 57

Resolution: metadata mismatch; doi, observed 2026-05-10T03:34:26.927602Z

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Observation 20ef6c1a-4992-43f1-88cf-1b05edd702a1 · 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: the stellar mass content of groups and clusters of galaxies

Reference 182

Resolution: verified exact; doi, observed 2026-05-10T02:06:36.940752Z

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Observation 645db287-9fe8-43fa-a0fd-794a1d780947 · 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: the stellar mass content of groups and clusters of galaxies

Reference 45

Resolution: verified exact; doi, observed 2026-05-10T02:17:13.144282Z

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Observation 7d7dc955-3ee7-4ec1-8a92-0704b423c5f7 · inbound

DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Proto-clusters cites this paper.

DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Proto-clusters First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 96

Resolution: metadata mismatch; doi, observed 2026-05-09T23:09:26.123764Z

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Observation d0290db1-7eae-45a6-a06c-b4bca7d11e3b · inbound

A graph-based Neural Network surrogate model for accelerating semi-analytical model of galaxy formation and evolution cites this paper.

A graph-based Neural Network surrogate model for accelerating semi-analytical model of galaxy formation and evolution First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 38

Resolution: metadata mismatch; doi, observed 2026-05-08T22:54:24.510502Z

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Observation b0f3805e-93b0-4319-a9d3-518ef41902f1 · 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: the stellar mass content of groups and clusters of galaxies

Reference 35

Resolution: metadata mismatch; doi, observed 2026-05-09T00:44:28.457493Z

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Observation edc807a6-6dc7-4155-b19b-e6f2ae878687 · 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: the stellar mass content of groups and clusters of galaxies

Reference 35

Resolution: metadata mismatch; doi, observed 2026-05-14T22:18:03.870279Z

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Observation 62b6a5d9-0ce6-4e8c-8330-ad30aa8d4e39 · 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: the stellar mass content of groups and clusters of galaxies

Reference 61

Resolution: metadata mismatch; doi, observed 2026-05-09T00:49:28.596512Z

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Observation 384b5adc-fb5a-4a40-946a-2db78b392781 · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:41:15.396590Z

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Observation 76758a43-9711-477a-a870-42c158c4212b · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 176

Resolution: metadata mismatch; doi, observed 2026-05-09T20:58:07.505979Z

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Observation 813b9f65-e2fb-4fcf-8807-7e110656840a · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 46

Resolution: verified exact; doi, observed 2026-05-08T17:58:53.353084Z

Source-reported events for the cited work

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Observation 76b39c2c-d247-4366-b7b4-1f3d0a93383f · inbound

The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence cites this paper.

The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 142

Resolution: metadata mismatch; doi, observed 2026-05-09T02:39:41.906688Z

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Observation c8a812ab-ab22-430d-bd19-e985ce40e9ac · inbound

The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence cites this paper.

The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 142

Resolution: metadata mismatch; doi, observed 2026-05-08T18:28:58.020806Z

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Observation 0e06dcd7-c77c-4554-8f27-4728a2e2a918 · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 73

Resolution: verified exact; doi, observed 2026-05-08T22:44:22.786847Z

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Observation 077ac33d-9980-4120-a61b-ef6cc3c51dd9 · inbound

Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model cites this paper.

Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 226

Resolution: metadata mismatch; doi, observed 2026-05-11T01:30:51.914756Z

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Observation fb88b6a9-fae1-45be-af10-add69b0a2a0c · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 92

Resolution: verified exact; doi, observed 2026-05-11T02:50:54.887705Z

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Observation e8972622-9718-4218-883e-82a5349e0d81 · 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: the stellar mass content of groups and clusters of galaxies

Reference 33

Resolution: metadata mismatch; doi, observed 2026-05-12T01:01:14.041004Z

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Observation ea6bf33b-1af3-49a4-90ad-8b9605c86070 · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-05-14T18:19:22.876866Z

Source-reported events for the cited work

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Observation bb06b74a-f2ce-4ad0-a12f-fd271de8df97 · inbound

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-05-19T16:17:39.163091Z

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Observation b5af15b7-b82d-409b-87ea-7d4dfadf20c6 · inbound

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: the stellar mass content of groups and clusters of galaxies

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-05-20T18:48:53.120871Z

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.

Observation e988ba62-eb60-4160-acb2-fc40d73b770c · 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: the stellar mass content of groups and clusters of galaxies

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:43:09.424819Z

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.

Observation 027dae24-498f-408f-b8e7-3dc9175db730 · inbound

Data-Efficient Neural Operator Training via Physics-Based Active Learning cites this paper.

Data-Efficient Neural Operator Training via Physics-Based Active Learning First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 11

Resolution: metadata mismatch; doi, observed 2026-05-21T05:33:58.087278Z

Source-reported events for the cited work

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Observation 8985354a-d8b7-4b8f-9a2c-6096229ef8ec · inbound

\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: the stellar mass content of groups and clusters of galaxies

Reference 240

Resolution: verified exact; local_arxiv, observed 2026-05-25T05:20:22.597116Z

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Observation ec7bb177-f719-40d5-8473-0f032ceecf83 · inbound

Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps cites this paper.

Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 113

Resolution: verified exact; doi, observed 2026-06-29T20:33:57.869417Z

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Observation 7adef3b7-ecef-448c-b2f2-ddaaa510df07 · 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: the stellar mass content of groups and clusters of galaxies

Reference 71

Resolution: metadata mismatch; doi, observed 2026-06-29T05:33:09.933547Z

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Observation e69ceb75-74ba-4da4-8277-3ce4569e9979 · inbound

Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots cites this paper.

Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 49

Resolution: metadata mismatch; doi, observed 2026-06-28T22:12:40.997939Z

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Observation ba45c237-9386-44cc-a4a6-1c59c99f38b6 · 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: the stellar mass content of groups and clusters of galaxies

Reference 116

Resolution: verified exact; local_arxiv, observed 2026-06-28T13:02:10.944539Z

Source-reported events for the cited work

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Observation eacefd9f-6db8-40e4-9d50-77e12a321280 · 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: the stellar mass content of groups and clusters of galaxies

Reference 145

Resolution: verified exact; local_arxiv, observed 2026-06-28T04:51:39.971815Z

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.

Observation db7134e7-d3b5-4308-952f-555d5a246836 · inbound

Mapping the star formation peak with LIGO A# and Next-Generation detectors cites this paper.

Mapping the star formation peak with LIGO A# and Next-Generation detectors First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 234

Resolution: verified exact; local_arxiv, observed 2026-06-28T05:11:40.062373Z

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.

Observation ecfcdfd4-2961-44ce-915f-818a0ced631a · 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: the stellar mass content of groups and clusters of galaxies

Reference 21

Resolution: metadata mismatch; local_arxiv, observed 2026-06-28T05:01:39.545620Z

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.

Observation 6a274bc8-f9f5-4318-ba1e-6e90ac7032fd · 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: the stellar mass content of groups and clusters of galaxies

Reference 174

Resolution: verified exact; local_arxiv, observed 2026-06-27T16:11:02.308137Z

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.

Observation 9e8b10ae-02e1-4d27-b564-99925375e31e · 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: the stellar mass content of groups and clusters of galaxies

Reference 15

Resolution: verified exact; local_arxiv, observed 2026-06-27T16:01:02.224366Z

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.

Observation 231f4e1a-cfbd-4f84-bedb-5a10fcd9d555 · inbound

Pressure-regulated feedback-modulated star formation as a subgrid model for galaxy formation simulations cites this paper.

Pressure-regulated feedback-modulated star formation as a subgrid model for galaxy formation simulations First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 40

Resolution: metadata mismatch; doi, observed 2026-06-27T15:51:00.768011Z

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.

Observation 33d9f755-e16b-4e34-add6-18fba6a1473e · inbound

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations cites this paper.

Learning the Universe: The Structure of Dust Attenuation Curves in Galaxy Simulations First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 125

Resolution: verified exact; local_arxiv, observed 2026-06-27T15:51:01.611007Z

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.

Observation 731cf596-b7c2-4cab-af47-a8bcc5d9afdb · 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: the stellar mass content of groups and clusters of galaxies

Reference 57

Resolution: verified exact; doi, observed 2026-06-27T19:31:11.083681Z

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.

Observation 2987a1ef-2b4a-4422-a6ed-256e301d9584 · inbound

AGN-driven BBH mergers: Black hole populations and hierarchical growth across the AGN parameter space cites this paper.

AGN-driven BBH mergers: Black hole populations and hierarchical growth across the AGN parameter space First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 72

Resolution: verified exact; local_arxiv, observed 2026-06-27T13:20:57.039837Z

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.

Observation 80261214-e73f-4f02-8c6b-5297c7d3a30d · inbound

Supermassive Black Hole Assembly from Heavy Seeds with Dynamical Friction in the BRAHMA Simulations: Implications for JWST, LISA, and the Local Universe cites this paper.

Supermassive Black Hole Assembly from Heavy Seeds with Dynamical Friction in the BRAHMA Simulations: Implications for JWST, LISA, and the Local Universe First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 103

Resolution: metadata mismatch; doi, observed 2026-06-27T07:00:40.112475Z

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.

Observation 1f520c64-3bc4-4156-8945-719739c164c4 · 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: the stellar mass content of groups and clusters of galaxies

Reference 26

Resolution: verified exact; doi, observed 2026-06-27T00:30:17.128431Z

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.

Observation 8a344011-8b09-440d-a894-3588167eb980 · 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: the stellar mass content of groups and clusters of galaxies

Reference 67

Resolution: verified exact; doi, observed 2026-06-26T16:59:36.075434Z

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.

Observation 9d7c6c5e-76ac-4116-b44c-b6886574f134 · inbound

Black Hole Occupation Fraction: Dependence on Black Hole Mass Threshold, Environment, Resolution and Redshift cites this paper.

Black Hole Occupation Fraction: Dependence on Black Hole Mass Threshold, Environment, Resolution and Redshift First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 46

Resolution: metadata mismatch; doi, observed 2026-06-26T08:29:12.771381Z

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.

Observation fb7c5e10-7082-44cd-8e66-2ada7389bdc3 · 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: the stellar mass content of groups and clusters of galaxies

Reference 222

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:59:08.666410Z

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.

Observation 758acacc-ba2c-4577-9388-ed08d183e064 · inbound

The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating cites this paper.

The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 161

Resolution: verified exact; doi, observed 2026-06-26T09:39:18.222061Z

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.

Observation ec69f3cf-5f6b-4ff9-baaf-5ab310df8824 · 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: the stellar mass content of groups and clusters of galaxies

Reference 42

Resolution: metadata mismatch; doi, observed 2026-06-25T23:58:42.827241Z

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.

Observation 1260dedc-6631-4369-b400-91904696176f · 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: the stellar mass content of groups and clusters of galaxies

Reference 61

Resolution: metadata mismatch; doi, observed 2026-06-25T23:38:41.905581Z

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.

Observation 9b78b0c2-1ec2-44a1-90ff-30fd3010ab82 · 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: the stellar mass content of groups and clusters of galaxies

Reference 68

Resolution: metadata mismatch; doi, observed 2026-06-26T06:39:04.643881Z

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.

Observation 17a7b860-8cc3-491d-87d3-62bc5c924247 · inbound

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium cites this paper.

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 118

Resolution: verified exact; local_arxiv, observed 2026-06-27T01:00:21.060166Z

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.

Observation 68d97a25-a551-4f99-998c-6263c79f650b · 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: the stellar mass content of groups and clusters of galaxies

Reference 35

Resolution: verified exact; doi, observed 2026-06-26T03:58:57.520142Z

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.

Observation 2b795099-176e-4042-a703-67b9fa0c6db2 · 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: the stellar mass content of groups and clusters of galaxies

Reference 244

Resolution: verified exact; local_arxiv, observed 2026-06-29T03:53:05.432346Z

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.

Observation cbe9f7df-e2b0-482a-a1f3-af3f664236a5 · 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: the stellar mass content of groups and clusters of galaxies

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-06-29T03:23:05.077063Z

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.

Observation 117df7ed-da79-4d14-9e31-0852e0211db7 · 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: the stellar mass content of groups and clusters of galaxies

Reference 246

Resolution: verified exact; local_arxiv, observed 2026-06-30T05:04:19.106510Z

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.

Observation f69a1880-d985-4f0d-bd38-620534d60bda · 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 First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 219

Resolution: verified exact; local_arxiv, observed 2026-07-01T04:25:21.711816Z

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.

Observation c801afef-4348-4a70-84ee-eae0c2fae9d7 · inbound

Fueling and feedback mechanisms at the nodes of the cosmic web cites this paper.

Fueling and feedback mechanisms at the nodes of the cosmic web First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-07-01T04:35:20.962278Z

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.

Observation f649989a-a41e-4b92-8e57-afcbf8015d7a · 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: the stellar mass content of groups and clusters of galaxies

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-07-02T09:36:49.032160Z

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.

Observation c32833ba-8dcf-4188-9a99-338bba043fca · 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: the stellar mass content of groups and clusters of galaxies

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-07-02T06:46:44.209581Z

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.

Observation 9e8c7ae0-2e29-430c-89fd-8d91f0bc05f9 · inbound

The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy cites this paper.

The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-07-03T08:37:46.052455Z

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.

Observation 2318aefa-d845-4546-b2a1-67fc48be1c4b · 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 IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-07-07T17:24:00.968575Z

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.

Observation 3fa1aa1a-9488-4ca0-a642-f0b791a9431f · 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: the stellar mass content of groups and clusters of galaxies

Reference 96

Resolution: metadata mismatch; doi, observed 2026-07-09T22:56:37.314047Z

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.

Observation d1fc4852-7f9f-4b9b-a824-75708e19d9cf · inbound

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers cites this paper.

Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 141

Resolution: verified exact; local_arxiv, observed 2026-07-09T20:06:29.280601Z

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.

Observation 740aa892-e4bb-4594-b0c7-63b433660129 · 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: the stellar mass content of groups and clusters of galaxies

Reference 25

Resolution: verified exact; local_arxiv, observed 2026-07-10T18:07:31.193530Z

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.

Observation 67f4bd80-861b-4972-be10-e50e9b296c01 · 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: the stellar mass content of groups and clusters of galaxies

Reference 32

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ceca321c-ca35-4a5a-a48c-d10387a81138 · inbound

Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations cites this paper.

Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-02T06:10:09.012138Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82dc9dcf-0410-4c7a-a6a4-39b94c2b56cc · 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: the stellar mass content of groups and clusters of galaxies

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:36.323178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d523228f-0cfa-4615-979f-a84699a456fd · 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: the stellar mass content of groups and clusters of galaxies

Reference 169

Resolution: unresolved; no resolver link, observed 2026-08-02T00:50:15.473474Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a99d06d0-3faf-4c41-8291-b419c131ce8d · inbound

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.

How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-01T23:42:37.978382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 81d3d487-b8e8-4150-8974-96b4676c23b2 · inbound

Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping cites this paper.

Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 143

Resolution: unresolved; no resolver link, observed 2026-08-01T12:40:13.382346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd1e3fa0-9eab-4c38-8c5f-ce9ecf2e1009 · 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 IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T08:26:01.151197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d9e050d1-ed9c-483e-801b-c354a827aa94 · 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: the stellar mass content of groups and clusters of galaxies

Reference 183

Resolution: unresolved; no resolver link, observed 2026-08-01T00:56:21.749084Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0d2e69de-d660-49d6-a177-6b988cfcfe54 · 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: the stellar mass content of groups and clusters of galaxies

Reference 91

Resolution: unresolved; no resolver link, observed 2026-07-31T22:07:32.568612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b58329fa-10e8-4d13-b5bf-ddeb3e033ed8 · 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: the stellar mass content of groups and clusters of galaxies

Reference 195

Resolution: unresolved; no resolver link, observed 2026-08-06T00:06:27.275387Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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