Pith. sign in

Paper Citation Record · LEDGER

A model for cosmological simulations of galaxy formation physics

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 34 inbound Pith citation observations for arXiv:1305.2913.

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

pith.paper-citation-record.v1
1305.2913 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 34 of 34 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 34 of 34 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T06:10:14.982419Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T18:07:31.173658Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

861
pith, observed 2026-07-10T18:07:31.173658Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7ea35ac0-e755-4794-99fb-b2c78073208a · inbound

COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase cites this paper.

COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase A model for cosmological simulations of galaxy formation physics

Reference 155

Resolution
verified exact
doi, observed 2026-05-18T19:41:47.684780Z

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=2026-05-18T19:37:22.323355Z digest=sha256:e6998b92e4208acf2a1dc1c5f07384564f8e64979557415d6ff2c3d1d9f1fdc2

Observation d0c06a1d-cc49-40d7-94c1-13e535eb127a · inbound

The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0 cites this paper.

The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0 A model for cosmological simulations of galaxy formation physics

Reference 155

Resolution
verified exact
doi, observed 2026-05-18T17:41:40.714707Z

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=2026-05-18T17:41:14.500802Z digest=sha256:5c05612399f26985d9dbe68e18b7fc62bc0dceee6e399e25241104f3f12658e7

Observation 3c19b7d0-2a91-4860-a057-10b07b83c761 · inbound

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift cites this paper.

Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift A model for cosmological simulations of galaxy formation physics

Reference 153

Resolution
metadata mismatch
doi, observed 2026-05-18T02:50:48.013015Z

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=2026-05-18T02:48:14.635035Z digest=sha256:b1acd9539065dea3376c57e08d3fb486bc38c5eaeeea2ad0112bfaf46d4913b3

Observation 07799f96-9531-4dde-9a3b-6e3fdb3a682f · inbound

First results of AMBRA: Abundant Seeds and Early Mergers as a Pathway to the First Massive Black Holes cites this paper.

First results of AMBRA: Abundant Seeds and Early Mergers as a Pathway to the First Massive Black Holes A model for cosmological simulations of galaxy formation physics

Reference 74

Resolution
metadata mismatch
doi, observed 2026-05-13T21:38:18.618987Z

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=2026-05-13T21:35:46.981945Z digest=sha256:800454a56867cf1eabb0ec30ad9b355747b09ce197edb97c8843d19209ea52f1

Observation 132ecf7c-0d9a-4301-9ae0-43f4ab3dfc22 · inbound

Self-regulated galaxy evolution within a self-consistently varying galaxy-wide IMF cites this paper.

Self-regulated galaxy evolution within a self-consistently varying galaxy-wide IMF A model for cosmological simulations of galaxy formation physics

Reference 2

Resolution
verified exact
doi, observed 2026-05-09T23:54:46.218399Z

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=2026-05-09T23:50:49.543693Z digest=sha256:1d181f80b4f591d6a19bbd1b25f602e42bda927c699d0391dca10fbceeec6225

Observation 1b22d49b-6604-4906-99c9-ed25a5fc12fd · 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 A model for cosmological simulations of galaxy formation physics

Reference 54

Resolution
metadata mismatch
doi, observed 2026-05-09T00:44:28.566091Z

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=2026-05-08T02:36:16.083207Z digest=sha256:8f3f2c5b847fb2e3ea5a2156a558c349062411d6eaf2f837ecc9674625ee6b1b

Observation 1367f840-03fb-4d3a-86d1-1575763d2af9 · 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 A model for cosmological simulations of galaxy formation physics

Reference 54

Resolution
metadata mismatch
doi, observed 2026-05-14T22:18:03.659040Z

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=2026-05-14T22:14:44.870705Z digest=sha256:67ca738d8e465520fc0148253bc06fbe375ec0b3af7bc0205b8ef2f8ab634f1d

Observation 6f9a8b6a-0d58-4078-96ad-ab479052fac8 · 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 A model for cosmological simulations of galaxy formation physics

Reference 239

Resolution
metadata mismatch
doi, observed 2026-05-09T20:58:07.215490Z

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=2026-05-09T20:54:41.217661Z digest=sha256:8e1f7ab53cbe9d020a1f29b605fcef85ecc49116f5c8566ca160e48f65e6a5f1

Observation b36af7e4-9473-4601-b33e-12dccd95bf11 · inbound

NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way cites this paper.

NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way A model for cosmological simulations of galaxy formation physics

Reference 126

Resolution
verified exact
doi, observed 2026-05-09T19:05:11.122731Z

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=2026-05-09T18:45:04.576956Z digest=sha256:fef4c6005c67e855ebad82d131774252951852a6477a933af5774528f2e57acf

Observation 8a207081-121f-45fe-a25e-10f276b7d908 · 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 A model for cosmological simulations of galaxy formation physics

Reference 65

Resolution
verified exact
doi, observed 2026-05-08T17:58:52.660019Z

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=2026-05-08T17:57:29.069633Z digest=sha256:c9b40447c77f143093e27fc7721584fdda3bbfdcd4f1d84fc360d4e6cb8ff48f

Observation ce397db5-19da-437c-b640-890a8afe7fa7 · inbound

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations cites this paper.

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations A model for cosmological simulations of galaxy formation physics

Reference 154

Resolution
metadata mismatch
doi, observed 2026-05-08T20:04:07.754273Z

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=2026-05-08T17:26:07.513278Z digest=sha256:0f380fac981d409fa0d0f1a9891554c62f2f740935a852ca3c68a0de9f1812b6

Observation 2fd65889-272b-4145-bf02-13bedefa6078 · 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 A model for cosmological simulations of galaxy formation physics

Reference 24

Resolution
verified exact
doi, observed 2026-05-11T01:30:52.139796Z

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=2026-05-11T00:53:14.584468Z digest=sha256:d0df825a16b13f9196d603d8c9217cfc985949ab6cb51ebedaae510a9db9a1fe

Observation f2ae5ed0-a2c4-4fed-bc4a-c21cbb2fe116 · inbound

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon cites this paper.

Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon A model for cosmological simulations of galaxy formation physics

Reference 157

Resolution
verified exact
doi, observed 2026-05-11T01:10:52.808992Z

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=2026-05-11T01:07:57.029580Z digest=sha256:f9d9087747c212f9309cd03fe525f56c04de6e53eaa91f8c59fafd52f85c5f35

Observation 4018ef04-4665-4b0c-b959-8240cd6e7a5e · 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 A model for cosmological simulations of galaxy formation physics

Reference 156

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:17:39.186031Z

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:a7cdb3efa6860316a3e938b6df769cd3a97c26adbd3aedebad8a8803b0420824

Observation 18524f9e-6621-4c04-8a26-e5fee4247c21 · inbound

The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization cites this paper.

The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization A model for cosmological simulations of galaxy formation physics

Reference 95

Resolution
verified exact
local_arxiv, observed 2026-05-20T08:43:09.043396Z

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=sha256:5553654dcafc38ada0104eb6d2a0d275ff73baf90f37500163b0508b305f37a7

Observation ac3ad04f-a1fb-4441-b97f-7cb0bc7a96d2 · 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 A model for cosmological simulations of galaxy formation physics

Reference 97

Resolution
metadata mismatch
doi, observed 2026-06-29T05:33:09.902170Z

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=2026-06-29T05:31:28.113100Z digest=sha256:67662d819059f8c56cb92b0ca31ff96b916612f8310e523632bf909bac52a8f3

Observation b3695b7e-ef07-4495-a20f-6e4a2b2293dd · inbound

The JADES Mass-Metallicity and Fundamental Metallicity Relations at $z\gtrsim2$ Using New High-Redshift Metallicity Calibrations cites this paper.

The JADES Mass-Metallicity and Fundamental Metallicity Relations at $z\gtrsim2$ Using New High-Redshift Metallicity Calibrations A model for cosmological simulations of galaxy formation physics

Reference 95

Resolution
metadata mismatch
doi, observed 2026-06-29T06:13:08.650856Z

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=2026-06-29T06:08:29.030525Z digest=sha256:61ca5d1b0e203ca63d555334668016ce85aaec63d413af3e87a02cff59d15314

Observation 4805d283-180b-4903-b3a1-c9e03d1d2bbe · inbound

COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $\mu$m Since $z=3$ cites this paper.

COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $\mu$m Since $z=3$ A model for cosmological simulations of galaxy formation physics

Reference 75

Resolution
metadata mismatch
doi, observed 2026-06-28T22:12:41.691780Z

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=2026-06-28T22:05:05.531469Z digest=sha256:642d74775988fb576d144731cf98b8360b550f7cf19831bc167332deb086b63c

Observation 43dd3c94-3f62-4673-ac43-7f365beec8e1 · 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 A model for cosmological simulations of galaxy formation physics

Reference 5

Resolution
verified exact
local_arxiv, observed 2026-06-27T16:11:02.254121Z

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=sha256:799e3981be8bcf280b8381843b78756eedb505e79eb55e7e73557b1399c79ddf

Observation 28619118-9bc2-4d03-8f94-79c261f3ab70 · 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 A model for cosmological simulations of galaxy formation physics

Reference 57

Resolution
metadata mismatch
doi, observed 2026-06-27T15:51:00.827915Z

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=2026-06-27T15:50:44.558873Z digest=sha256:71d177f2f04b6f1af3e9e0a770ac992b1c3b988a4b9efd99202e5848ffb97fe3

Observation 6dc5fde8-58c8-4ca0-85de-0fb093b072fa · 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 A model for cosmological simulations of galaxy formation physics

Reference 68

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:21:00.475788Z

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:f6e0a237dca071e821da43ca2b8ce7b8566a32d9d22c323a9991c9736c55390f

Observation 6b55e047-dcd6-477d-8683-87825f97ca93 · inbound

Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth cites this paper.

Learning the Universe at High Redshifts: Impact of Accretion Modeling on Early Black Hole Growth A model for cosmological simulations of galaxy formation physics

Reference 90

Resolution
metadata mismatch
doi, observed 2026-06-27T17:21:07.092051Z

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=2026-06-27T15:45:43.759962Z digest=sha256:03f1b61bee7ed2fc913cd06d311d55ec4d14bf3936224b23812ebb0666153c59

Observation a129c2fd-6215-4702-a6c9-ee08ad808b53 · 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 A model for cosmological simulations of galaxy formation physics

Reference 94

Resolution
verified exact
doi, observed 2026-06-27T20:31:14.788565Z

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:e3d35f0cf75e4e85feb7e7a153cc18d52ae6989bb121aae56b38e9a56ff4d8a5

Observation af4f39fc-4f4e-427a-8d4f-37a108eead16 · 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 A model for cosmological simulations of galaxy formation physics

Reference 131

Resolution
metadata mismatch
doi, observed 2026-06-27T07:00:40.207967Z

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=2026-06-27T06:55:11.433036Z digest=sha256:e4910b214cdd4550da5aa1a4f82dac7a1b268fb9a8658cacefb7a6e060fd7455

Observation 4b9540ac-25e9-4705-a680-55cf7bd37237 · 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 A model for cosmological simulations of galaxy formation physics

Reference 42

Resolution
verified exact
doi, observed 2026-06-27T00:30:17.055648Z

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:b67ca1b432fdd5ccaa7171c8221e4fa44034e921578ce51b63fe58d4551d6aa5

Observation 37a6778b-39aa-485c-b4b6-4d8358ae5d30 · inbound

The Lumina Project: Intergalactic Clumping and Recombination Sinks cites this paper.

The Lumina Project: Intergalactic Clumping and Recombination Sinks A model for cosmological simulations of galaxy formation physics

Reference 83

Resolution
verified exact
local_arxiv, observed 2026-06-26T23:40:14.833798Z

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=sha256:772fe2ef64cc7221fdc8a5bc028f71e33f8be5a809d7a85e1f95fe719fcc3f31

Observation 6616c7ca-f369-4ee0-9dfe-209e544dc708 · inbound

The Lifecycle and Emission Properties of PAHs in Cosmological Hydrodynamic Galaxy Formation Simulations cites this paper.

The Lifecycle and Emission Properties of PAHs in Cosmological Hydrodynamic Galaxy Formation Simulations A model for cosmological simulations of galaxy formation physics

Reference 161

Resolution
verified exact
doi, observed 2026-06-26T16:29:36.240764Z

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=2026-06-26T16:22:24.087328Z digest=sha256:344eb00a2d1d2645d915e8e9fd64b671057e9378cf57c739c789f9ffe82e99eb

Observation f0c45c98-a5b1-4dba-8bfb-023d8cea39a4 · 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 A model for cosmological simulations of galaxy formation physics

Reference 224

Resolution
verified exact
doi, observed 2026-06-26T09:39:18.241604Z

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=2026-06-26T07:50:38.631331Z digest=sha256:287e4a8ecb86ae33295ed9373bccc5f13b268ee858dcc965d17d43965319b4fb

Observation c9408793-ebf9-4aff-9120-c0f59fd04735 · 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 A model for cosmological simulations of galaxy formation physics

Reference 83

Resolution
metadata mismatch
doi, observed 2026-06-25T23:38:41.864871Z

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=sha256:9afd2b56241d1c71f206d5c36e19cdbf1701f2ab46e5c6f12fc5be33b4382bdb

Observation bd7cd06c-5dc5-4920-bc79-e695ab0ffac0 · inbound

Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations cites this paper.

Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations A model for cosmological simulations of galaxy formation physics

Reference 280

Resolution
verified exact
local_arxiv, observed 2026-06-25T23:48:42.929377Z

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:f32b67b0db42f28dfee3fd7c51ea329d86a536b86fa1fd2b349f6aa795b1189a

Observation 4265427e-3c21-432f-bcab-ae9d6d797402 · inbound

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters cites this paper.

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters A model for cosmological simulations of galaxy formation physics

Reference 112

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:45:14.269062Z

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=sha256:8d348ab291802e9eaf6d7720be3b5a046604fe928c7a93be88c647e88aa0326e

Observation e1c439ef-35d7-4d88-bc05-5c740ea8e312 · 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 A model for cosmological simulations of galaxy formation physics

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-07-10T18:07:31.175054Z

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:e03da25bb8f4192076e186e5218eb74f1404fb62df58d6df16fb5e46ce94a43d

Observation 3535e302-db24-4f94-99da-3840d299a9e9 · 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 A model for cosmological simulations of galaxy formation physics

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-02T06:10:14.982419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:10:14.982419Z digest=sha256:9263f715c6ae244f9a960c8418367de35a9f790cb789be55b6890a8932de0254

Observation 4b9b1063-fa7d-4225-ad8e-75a52addd029 · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ A model for cosmological simulations of galaxy formation physics

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:35.531519Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:35.531519Z digest=sha256:bbcd6c1c301ff9a50a0ad9285dca260a8fdfc67a2e977278918d718f43dcd055